This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d
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
NSVS J0541490-210310,2461126.6223,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0541490-210310 20260327.1223 12.80CV 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/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:48.78 -21:03:08.4 ;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_Lep-01-Q2b1x1_2026-01-20_22-22-49_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20_00sec_-10_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20_00sec_-10_00C_LIGHT_0063_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.1223 2461126.6223 12.07 04:54:52.08 -22:01:21.3
221.90603 -34.94341 galactic Eri Second-epoch detections are separated by 1.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2973302887182219904 | 04:54:52.07 -22:01:21.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.629+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.1223* 04 54 52.08 -22 01 21.3 12.1 U Eri 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
Gaia DR3 2973302887182219904,2461126.6223,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2973302887182219904 20260327.1223 12.07CV 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/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:52.08 -22:01:21.3 ;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_Lep-01-Q2b1x1_2026-01-20_22-22-49_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20_00sec_-10_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20_00sec_-10_00C_LIGHT_0063_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20_00sec_-10_00C_LIGHT_0062_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: 2461061.68263212 21.01.2026 04:22:49.415 /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
First image: 2461061.68263212 21.01.2026 04:22:49.415 /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
Last image: 2461126.62292201 27.03.2026 02:56:50.462 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.93
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): 8483
Objects passed selection criteria: 8461
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 6775
Average stars matched: 6632 (97.8893 %)
Memory usage VmPeak: 114868 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 22:02:57 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: 2461061.68263212 21.01.2026 04:22:49.415 /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
First image: 2461061.68263212 21.01.2026 04:22:49.415 /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
Last image: 2461126.62292201 27.03.2026 02:56:50.462 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 77
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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: 14 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): 52917
Objects passed selection criteria: 52818
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 43398.5
Average stars matched: 42048.8 (96.8899 %)
Memory usage VmPeak: 155788 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 22:04:15 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
SExtractor catalog cache: saved Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat to cache
SExtractor catalog cache: saved Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.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/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.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: 2461126.62162547
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits exists and is non-empty
Saving wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits to local_wcs_cache/
'wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits' -> 'local_wcs_cache/wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits'
wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits exists and is non-empty
Saving wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits to local_wcs_cache/
'wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits' -> 'local_wcs_cache/wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits'
wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits exists and is non-empty
Saving wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits to local_wcs_cache/
'wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits'
wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits exists and is non-empty
Saving wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits to local_wcs_cache/
'wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits' -> 'local_wcs_cache/wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.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 05:20:00.014 -18:00:30.48
Second-epoch image center 05:20:01.138 -18:00:21.95
Angular distance between the image centers 0.01 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 05:20:00.014 -18:00:30.48
Second-epoch image center 05:19:58.865 -18:00:20.23
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 05:20:01.138 -18:00:21.95
Second-epoch second image center 05:19:58.865 -18:00:20.23
Angular distance between the image centers 0.00902 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/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits &> /tmp/tmp.PC5Xs1Q5Qg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits &> /tmp/tmp.a6rtoradjG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits &> /tmp/tmp.DIgFB5T5zn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits &> /tmp/tmp.lrNHfn2PMm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
Calibrating the magnitude scale
Found non-empty wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.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_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.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_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat
Found non-empty wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat
The reference image (wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits) and catalog (wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat) found
'wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.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 7478 out of 10289 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.858404
a=0.000000 b=1.000000 c=22.858404
From vast_summary.log: estimated ref. image limiting mag.: -7.93
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.93
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.93
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
2.1 pix Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
2.4 pix fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
2.4 pix fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
Limiting magnitude estimates:
14.9 mag. Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
14.9 mag. Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
13.9 mag. fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
13.9 mag. fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.PC5Xs1Q5Qg (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits' -> 'wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
WCS_IMAGE_NAME=wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
WCS-calibrated image found: wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
Checking if the catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat corresponding to the image wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits alredy exist and is non-empty...
Catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat corresponding to the image wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
WCS catalog name: wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=785, passed=10289
Got 10289 stars (including 9485 good ones) from the SExtractor catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat
util/solve_plate_with_UCAC5 got 10289 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 972 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: 0.31"
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 972 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: 0.30"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits -region wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.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.a6rtoradjG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits' -> 'wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
Checking if the catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
WCS catalog name: wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=802, passed=10221
Got 10221 stars (including 9407 good ones) from the SExtractor catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat
util/solve_plate_with_UCAC5 got 10221 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 972 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 972 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: 0.29"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits -region wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.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.DIgFB5T5zn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
Checking if the catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
WCS catalog name: wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=381, passed=5218
Got 5218 stars (including 4831 good ones) from the SExtractor catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 5218 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits -region wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.lrNHfn2PMm (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=407, passed=5179
Got 5179 stars (including 4771 good ones) from the SExtractor catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat
util/solve_plate_with_UCAC5 got 5179 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 972 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits -region wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.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_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits'
Saving fully-calibrated image wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits'
Saving fully-calibrated image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits'
Saving fully-calibrated image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits'
Preparing the HTML report for the field Lep-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20513_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 20513_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:25:43.61 -14:23:33.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03498_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 03498_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:18:20.06 -16:21:07.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Lep-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
SExtractor catalog cache: saved Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat to cache
SExtractor catalog cache: saved Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
Creating symlink local_wcs_cache/wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
Creating symlink local_wcs_cache/wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
Creating symlink local_wcs_cache/wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.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_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits exists and is non-empty
wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits exists and is non-empty
wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits exists and is non-empty
wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.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 05:20:00.014 -18:00:30.48
Second-epoch image center 05:20:01.138 -18:00:21.95
Angular distance between the image centers 0.01 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 05:20:00.014 -18:00:30.48
Second-epoch image center 05:19:58.865 -18:00:20.23
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 05:20:01.138 -18:00:21.95
Second-epoch second image center 05:19:58.865 -18:00:20.23
Angular distance between the image centers 0.00902 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/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits &> /tmp/tmp.IOktoEYkxC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits &> /tmp/tmp.pJdU7hmZTN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits &> /tmp/tmp.mYq0QJr0Me
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits &> /tmp/tmp.5VgSLft2Jy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
Calibrating the magnitude scale
Found non-empty wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.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_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.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_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat
Found non-empty wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat
The reference image (wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits) and catalog (wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat) found
'wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.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 8117 out of 62896 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.718315
a=0.000000 b=1.000000 c=22.718315
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
2.0 pix Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
2.4 pix fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
2.3 pix fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
Limiting magnitude estimates:
15.1 mag. Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
15.1 mag. Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
14.1 mag. fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
14.1 mag. fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.IOktoEYkxC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits' -> 'wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
WCS_IMAGE_NAME=wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
WCS-calibrated image found: wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
Checking if the catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat corresponding to the image wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits alredy exist and is non-empty...
Catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat corresponding to the image wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
WCS catalog name: wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=3506, passed=62885
Got 62885 stars (including 59273 good ones) from the SExtractor catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat
util/solve_plate_with_UCAC5 got 62885 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits -region wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.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.pJdU7hmZTN (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits' -> 'wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
Checking if the catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
WCS catalog name: wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=3513, passed=63305
Got 63305 stars (including 59680 good ones) from the SExtractor catalog wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat
util/solve_plate_with_UCAC5 got 63305 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits -region wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.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.mYq0QJr0Me (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
Checking if the catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
WCS catalog name: wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1475, passed=32161
Got 32161 stars (including 30638 good ones) from the SExtractor catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 32161 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits -region wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5VgSLft2Jy (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1470, passed=32259
Got 32259 stars (including 30750 good ones) from the SExtractor catalog wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat
util/solve_plate_with_UCAC5 got 32259 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits -region wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.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_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/wcs_Lep-01-Q2b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits
Saving fully-calibrated image wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/wcs_Lep-01-Q2b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits
Saving fully-calibrated image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-54-58_20.00sec_-10.00C_LIGHT_0062.fits
Saving fully-calibrated image wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lep-01-Q2b1x1_220039_TTUQ2b1x1_8730_xbur9i6d/wcs_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063.fits
Preparing the HTML report for the field Lep-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out16473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77808.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out47765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52205.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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 77480_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77480_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:17:36.13 -19:05:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77483_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77483_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:19:21.77 -19:03:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77485_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77485_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:35:36.64 -21:28:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77489_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77489_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:19:18.26 -18:30:33.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 77544_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77544_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 04:54:16.00 -21:52:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.67, MAG_FAINT_SEARCH_LIMIT=11.65)GAIADR2_OUTPUT=# 1.680 2973319654732337792 073.56621956665 -21.86821361992 10.2811 9.5736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77582_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77582_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 04:54:08.58 -20:56:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77715_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77715_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:17:38.15 -15:14:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77745_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77745_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:15:43.16 -22:01:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77750_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77750_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:17:00.00 -14:56:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77791_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77791_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:13:27.69 -17:06:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77808_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77808_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:30:31.78 -19:39:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.740 2968753623462475776 082.63265449586 -19.66471067929 13.2228 12.8117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77856_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77856_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:16:53.98 -14:56:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.049 2983558650609575040 079.22433027985 -14.94205485049 13.2269 12.5557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77893_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77893_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 04:54:07.38 -22:03:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.257 2973304089772966144 073.53094923775 -22.06417588631 12.6110 12.1364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77981_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 77981_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:44:04.25 -15:48:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.580 2995263776522010752 086.01768946448 -15.80670030345 13.5446 12.8520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78012_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 78012_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:37:49.95 -15:48:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52205_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
Preparing report for the candidate 52205_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
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Considering the candidate 59556_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 59556_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:13:44.24 -20:03:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21711_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 21711_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:18:20.06 -16:21:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47765_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
Preparing report for the candidate 47765_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
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Considering the candidate 16473_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 16473_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 05:03:41.86 -15:32:53.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)
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Considering the candidate 10019_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063
The candidate 10019_fd_Lep-01-Q2b1x1_2026-03-26_21-56-50_20.00sec_-10.00C_LIGHT_0063 did not pass the final checks