This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.8843,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.3843 12.21CV 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/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:03:30.97 -14:26:36.2 ;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_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.8843,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.3843 12.77CV 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/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:46:00.98 -09:57:16.3 ;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_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.8843,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.3843 14.32CV 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/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:26:32.39 -09:42:41.8 ;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_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.8843,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.3843 14.48CV 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/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:31:47.99 -12:14:51.0 ;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_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20_00sec_-15_00C_LIGHT_0445_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: 2461059.01791420 18.01.2026 12:25:37.787 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
First image: 2461059.01791420 18.01.2026 12:25:37.787 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Last image: 2461093.88465544 22.02.2026 09:13:44.230 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.83
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: 5 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): 6604
Objects passed selection criteria: 6601
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 6429.25
Average stars matched: 6327.25 (98.4135 %)
Memory usage VmPeak: 112668 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 03:26:03 CST 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: 2461059.01791420 18.01.2026 12:25:37.787 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
First image: 2461059.01791420 18.01.2026 12:25:37.787 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Last image: 2461093.88465544 22.02.2026 09:13:44.230 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.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.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 15 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 43955
Objects passed selection criteria: 43842
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 42387.5
Average stars matched: 41090.5 (96.9401 %)
Memory usage VmPeak: 143944 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 03:27:33 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
SExtractor catalog cache: saved Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.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/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.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: 2461093.88396811
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits exists and is non-empty
Saving wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits to local_wcs_cache/
'wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits' -> 'local_wcs_cache/wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits'
wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits exists and is non-empty
Saving wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits to local_wcs_cache/
'wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits' -> 'local_wcs_cache/wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits'
wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits'
wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.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 14:34:18.609 -09:59:52.98
Second-epoch image center 14:34:18.367 -10:00:03.36
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:18.609 -09:59:52.98
Second-epoch image center 14:34:21.145 -10:00:32.83
Angular distance between the image centers 0.02 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 14:34:18.367 -10:00:03.36
Second-epoch second image center 14:34:21.145 -10:00:32.83
Angular distance between the image centers 0.01403 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/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits &> /tmp/tmp.Zb9nRMSVNQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits &> /tmp/tmp.Z9sQRIhAG0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits &> /tmp/tmp.hHxY7ZUeCb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits &> /tmp/tmp.r1hC83EiV3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
Found non-empty wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
The reference image (wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits) and catalog (wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat) found
'wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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 3807 out of 6729 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.871094
a=0.000000 b=1.000000 c=22.871094
From vast_summary.log: estimated ref. image limiting mag.: -7.83
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
____ 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 Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
2.1 pix Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
2.3 pix fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
2.3 pix fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
Limiting magnitude estimates:
15.0 mag. Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
15.0 mag. Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
14.9 mag. fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
14.9 mag. fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Zb9nRMSVNQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits' -> 'wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS-calibrated image found: wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Checking if the catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS catalog name: wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=516, passed=6729
Got 6729 stars (including 6204 good ones) from the SExtractor catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 6729 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.31"
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 971 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: 0.29"
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_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits -region wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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.Z9sQRIhAG0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits' -> 'wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS-calibrated image found: wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
Checking if the catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS catalog name: wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=536, passed=6698
Got 6698 stars (including 6151 good ones) from the SExtractor catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
util/solve_plate_with_UCAC5 got 6698 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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: 0.28"
Estimated accuracy of the plate solution: 0.27"
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_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits -region wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.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.hHxY7ZUeCb (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_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.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_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
Checking if the catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
WCS catalog name: wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=495, passed=6221
Got 6221 stars (including 5715 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat
util/solve_plate_with_UCAC5 got 6221 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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: 0.36"
Estimated accuracy of the plate solution: 0.35"
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_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits -region wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.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.r1hC83EiV3 (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_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.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_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
Checking if the catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
WCS catalog name: wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=493, passed=6248
Got 6248 stars (including 5748 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat
util/solve_plate_with_UCAC5 got 6248 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 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: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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: 0.36"
Estimated accuracy of the plate solution: 0.35"
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_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits -region wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.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_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits'
Saving fully-calibrated image wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits'
Preparing the HTML report for the field Lib-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20285.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 20285_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 20285_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:21:05.40 -06:55:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 0.398 3639906997208202752 215.27256128460 -06.92459238888 11.5749 11.0993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20290_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 20290_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:46:18.38 -07:15:50.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Lib-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
SExtractor catalog cache: saved Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Creating symlink local_wcs_cache/wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.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_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits exists and is non-empty
wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits exists and is non-empty
wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits exists and is non-empty
wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.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 14:34:18.609 -09:59:52.98
Second-epoch image center 14:34:18.367 -10:00:03.36
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:18.609 -09:59:52.98
Second-epoch image center 14:34:21.145 -10:00:32.83
Angular distance between the image centers 0.02 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 14:34:18.367 -10:00:03.36
Second-epoch second image center 14:34:21.145 -10:00:32.83
Angular distance between the image centers 0.01403 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/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits &> /tmp/tmp.AIDBkiCi7q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits &> /tmp/tmp.8JwnaORCmx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits &> /tmp/tmp.DOHYyyWWYp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits &> /tmp/tmp.eVIcAV6oVL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
Found non-empty wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
The reference image (wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits) and catalog (wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat) found
'wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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 3945 out of 44688 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.729906
a=0.000000 b=1.000000 c=22.729906
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.19
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.19
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 24 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
1.9 pix Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
2.1 pix fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
2.1 pix fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
Limiting magnitude estimates:
15.2 mag. Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
15.2 mag. Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
15.0 mag. fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
15.0 mag. fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.AIDBkiCi7q (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits' -> 'wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS-calibrated image found: wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Checking if the catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS catalog name: wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1825, passed=44675
Got 44675 stars (including 42782 good ones) from the SExtractor catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 44675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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: 0.29"
Estimated accuracy of the plate solution: 0.27"
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_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits -region wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q1b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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.8JwnaORCmx (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits' -> 'wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS-calibrated image found: wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
Checking if the catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS catalog name: wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1859, passed=44694
Got 44694 stars (including 42756 good ones) from the SExtractor catalog wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
util/solve_plate_with_UCAC5 got 44694 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.26"
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_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits -region wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q1b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.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.DOHYyyWWYp (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_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.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_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
Checking if the catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
WCS catalog name: wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1736, passed=40694
Got 40694 stars (including 38902 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat
util/solve_plate_with_UCAC5 got 40694 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 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_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits -region wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.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.eVIcAV6oVL (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_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.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_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
Checking if the catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
WCS catalog name: wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1708, passed=40632
Got 40632 stars (including 38855 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat
util/solve_plate_with_UCAC5 got 40632 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 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_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits -region wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.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_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.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_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-12-44_20.00sec_-15.00C_LIGHT_0445.fits
Saving fully-calibrated image wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.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_2026-02-22_CI_Lib-01-Q1b1x1_031430_TTUQ1b1x1_2241_h66j8oXf/wcs_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446.fits
Preparing the HTML report for the field Lib-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53663.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 53505_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53505_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:05:20.12 -09:37:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.681 3615067792586081280 211.33427770812 -09.62124465600 14.0311 13.5034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53510_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53510_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:57:45.65 -06:50:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.797 6333449007650654592 224.44067919693 -06.83451940868 14.5153 13.9573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53516_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53516_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:35:34.76 -07:00:37.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)
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Considering the candidate 53517_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53517_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:15:33.11 -10:32:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53518_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53518_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:06:28.09 -07:16:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 4.253 3640349241400674816 211.61803231257 -07.27640587870 14.2706 13.8042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53521_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53521_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:55:40.03 -07:23:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.467 6333399628410535808 223.91709401351 -07.39130387681 13.0278 12.3406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53534_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
Preparing report for the candidate 53534_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
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Considering the candidate 53539_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
Preparing report for the candidate 53539_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
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Considering the candidate 53545_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53545_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:52:03.18 -07:22:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53557_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53557_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 15:05:08.87 -05:20:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.561 6335522136824786816 226.28705322652 -05.34887395817 13.5906 12.9313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53573_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53573_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:22:18.31 -11:48:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53581_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53581_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 15:01:46.26 -13:54:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.398 6311843466726282368 225.44292996404 -13.90206902334 14.2731 13.4309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53589_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53589_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:58:00.25 -13:03:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 0.763 6312190873744449792 224.50096305564 -13.05714197379 14.4966 13.9415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53593_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53593_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:49:48.27 -06:32:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53594_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53594_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 15:05:00.69 -12:48:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 0.998 6312389992724608128 226.25309287619 -12.80184487942 14.4384 13.9348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53595_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53595_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 15:05:02.24 -07:27:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53607_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53607_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:59:26.95 -13:15:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53609_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
Preparing report for the candidate 53609_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
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Considering the candidate 53627_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53627_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:52:35.02 -14:43:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.788 6310400632592547200 223.14633906828 -14.72303248508 14.3670 13.8656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53628_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53628_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:54:23.53 -05:26:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 0.381 6337162264576006144 223.59794081654 -05.44913287122 14.6828 14.0846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53648_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53648_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:52:13.73 -14:08:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.720 6310508762689387648 223.05754509423 -14.13693214670 14.4891 13.9537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53663_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
Preparing report for the candidate 53663_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
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Considering the candidate 53724_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 53724_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks
**** FOUND 14:59:37.35 -12:21:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.117 6312342851163762560 224.90593520750 -12.36082154492 14.3628 13.6919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 39330_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446
The candidate 39330_fd_Lib-01-Q1b1x1_2026-02-22_03-13-44_20.00sec_-14.90C_LIGHT_0446 did not pass the final checks