This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz
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!
TCP 2026 02 27.1817* 10 38 24.84 +19 08 42.2 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6817,12.63,0.05,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 20260227.1817 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:38:24.84 +19:08:42.2 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 40 31.85 +21 28 38.0 13.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6817,13.53,0.05,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 20260227.1817 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:40:31.85 +21:28:38.0 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 01 30.35 +23 42 45.6 13.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6817,13.52,0.05,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 20260227.1817 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:01:30.35 +23:42:45.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 09 37 07.46 +24 36 05.4 13.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6817,13.73,0.05,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 20260227.1817 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:37:07.46 +24:36:05.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1817 2461098.6817 13.77 09:38:32.36 +19:24:48.5
212.17384 45.29768 galactic Leo Second-epoch detections are separated by 5.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 633645875323090944 | 09:38:35.59 +19:24:46.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 09 38 32.36 +19 24 48.5 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 633645875323090944,2461098.6817,13.77,0.05,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
Gaia DR3 633645875323090944 20260227.1817 13.77CV 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:38:32.36 +19:24:48.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 08 50.60 +19 32 36.3 13.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6817,13.87,0.05,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 20260227.1817 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:08:50.60 +19:32:36.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 09 42.63 +18 45 23.2 14.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6817,14.16,0.05,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 20260227.1817 14.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:09:42.63 +18:45:23.2 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 00 02.39 +22 37 52.8 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6817,14.36,0.05,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 20260227.1817 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:00:02.39 +22:37:52.8 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 16 25.62 +17 41 46.1 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6817,14.41,0.05,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 20260227.1817 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:16:25.62 +17:41:46.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 09 58 05.41 +21 46 54.1 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6817,14.43,0.05,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 20260227.1817 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:58:05.41 +21:46:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_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: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
First image: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Last image: 2461098.68193823 27.02.2026 04:21:49.463 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.80
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5038
Objects passed selection criteria: 5037
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: 4748.25
Average stars matched: 4678 (98.5205 %)
Memory usage VmPeak: 111560 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 Thu Feb 26 22:29:23 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: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
First image: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Last image: 2461098.68193823 27.02.2026 04:21:49.463 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 86
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: 10 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): 29594
Objects passed selection criteria: 29543
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: 28203
Average stars matched: 27556.5 (97.7077 %)
Memory usage VmPeak: 132632 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 Thu Feb 26 22:30:06 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.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: 2461098.68151192
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits exists and is non-empty
Saving wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits to local_wcs_cache/
'wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits'
wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits exists and is non-empty
Saving wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits to local_wcs_cache/
'wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits'
wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits'
wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:13.854 +22:00:03.61
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:12.583 +22:00:03.80
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:09:13.854 +22:00:03.61
Second-epoch second image center 10:09:12.583 +22:00:03.80
Angular distance between the image centers 0.00491 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits &> /tmp/tmp.d8HI2D3Pam
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits &> /tmp/tmp.5hqgpxY305
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits &> /tmp/tmp.q3KqY4fngm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits &> /tmp/tmp.dKKZdPvA5S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Found non-empty wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
The reference image (wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits) and catalog (wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat) found
'wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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 3674 out of 5334 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.866726
a=0.000000 b=1.000000 c=22.866726
From vast_summary.log: estimated ref. image limiting mag.: -7.80
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
2.1 pix Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
2.0 pix fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
2.0 pix fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
Limiting magnitude estimates:
15.1 mag. Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
15.1 mag. Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
14.7 mag. fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
14.7 mag. fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (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.d8HI2D3Pam (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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=391, passed=5334
Got 5334 stars (including 4935 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
util/solve_plate_with_UCAC5 got 5334 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 907 stars left (next iteration limit 997)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits -region wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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.5hqgpxY305 (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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=401, passed=5315
Got 5315 stars (including 4910 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
util/solve_plate_with_UCAC5 got 5315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 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 - 910 stars left (next iteration limit 1001)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits -region wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.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.q3KqY4fngm (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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=375, passed=4233
Got 4233 stars (including 3854 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat
util/solve_plate_with_UCAC5 got 4233 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 907 stars left (next iteration limit 997)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits -region wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.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.dKKZdPvA5S (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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=364, passed=4220
Got 4220 stars (including 3854 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 4220 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 908 stars left (next iteration limit 998)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits -region wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.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_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits'
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits'
Preparing the HTML report for the field Leo-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20278_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 20278_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 10:12:00.07 +19:22:00.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03624_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 03624_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 10:07:43.44 +23:59:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05268_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 05268_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 10:02:41.12 +26:41:35.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Leo-02-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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Creating symlink local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits exists and is non-empty
wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits exists and is non-empty
wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits exists and is non-empty
wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:13.854 +22:00:03.61
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:12.583 +22:00:03.80
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:09:13.854 +22:00:03.61
Second-epoch second image center 10:09:12.583 +22:00:03.80
Angular distance between the image centers 0.00491 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits &> /tmp/tmp.hZHktm5vpN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits &> /tmp/tmp.7zakXKrTvg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits &> /tmp/tmp.qlXbXOCWA4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits &> /tmp/tmp.PFGkdRCXWc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Found non-empty wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
The reference image (wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits) and catalog (wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat) found
'wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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 3822 out of 30893 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.745787
a=0.000000 b=1.000000 c=22.745787
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.21
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 62 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
2.0 pix Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
1.9 pix fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
2.0 pix fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
Limiting magnitude estimates:
15.2 mag. Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
15.2 mag. Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
14.9 mag. fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
14.9 mag. fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.3 (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.hZHktm5vpN (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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1127, passed=30880
Got 30880 stars (including 29685 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
util/solve_plate_with_UCAC5 got 30880 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 902 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits -region wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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.7zakXKrTvg (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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1098, passed=31047
Got 31047 stars (including 29892 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
util/solve_plate_with_UCAC5 got 31047 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 905 stars left (next iteration limit 995)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits -region wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.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.qlXbXOCWA4 (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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=875, passed=25880
Got 25880 stars (including 24953 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat
util/solve_plate_with_UCAC5 got 25880 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 902 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits -region wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.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.PFGkdRCXWc (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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=888, passed=25733
Got 25733 stars (including 24800 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 25733 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 903 stars left (next iteration limit 993)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits -region wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.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_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.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_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits
Preparing the HTML report for the field Leo-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52193.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 6s
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Considering the candidate 52107_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52107_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 09:52:33.26 +17:40:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 0.164 620282204840716672 148.13854698323 +17.66744280623 12.6059 11.9458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52108_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52108_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 52109_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52109_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 52111_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
Preparing report for the candidate 52111_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
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Considering the candidate 52112_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52112_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 52114_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52114_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 52115_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52115_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 09:51:55.58 +24:21:46.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52116_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52116_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 52119_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52119_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 52121_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52121_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 10:39:56.26 +18:04:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.272 3986009068375760896 159.98422940965 +18.07807766649 13.5458 12.9792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52122_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
Preparing report for the candidate 52122_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
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Considering the candidate 52123_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52123_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52124_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
Preparing report for the candidate 52124_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
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Considering the candidate 52126_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52126_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 10:20:25.29 +25:41:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.306 726980187589813760 155.10502495157 +25.68384573765 13.7134 13.1181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52127_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52127_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 09:50:55.85 +20:47:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.331 628064994818532608 147.73310338325 +20.78698399144 13.5849 12.9806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52129_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
Preparing report for the candidate 52129_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
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Considering the candidate 52131_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52131_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 52132_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52132_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52133_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
Preparing report for the candidate 52133_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
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Considering the candidate 52134_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
Preparing report for the candidate 52134_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
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Considering the candidate 52139_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52139_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 52141_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52141_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 52142_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52142_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 52143_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52143_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52145_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52145_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 52147_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52147_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 52148_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
Preparing report for the candidate 52148_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
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Considering the candidate 52149_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52149_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 52150_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52150_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 52151_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52151_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 52152_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52152_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 52153_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52153_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 52154_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52154_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 52156_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52156_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 52157_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52157_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 52159_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52159_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 52160_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52160_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 52162_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52162_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 52164_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52164_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 52165_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52165_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 52166_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52166_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 09:52:43.86 +21:38:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.780 640234179061099520 148.18328059613 +21.64285408380 14.5510 13.9157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52167_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52167_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 52168_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52168_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 52169_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52169_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 52170_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52170_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52171_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52171_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 09:37:48.35 +20:25:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52175_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52175_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 52176_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52176_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52178_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
Preparing report for the candidate 52178_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
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Considering the candidate 52180_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
Preparing report for the candidate 52180_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
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Considering the candidate 52183_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52183_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 09:54:53.29 +26:42:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52185_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52185_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 52186_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52186_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52190_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52190_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52193_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
Preparing report for the candidate 52193_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
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Considering the candidate 52195_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52195_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 52196_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52196_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 10:40:31.85 +27:03:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.845 725070301532360320 160.13285049906 +27.05285786389 14.6002 14.0592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52198_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52198_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52203_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52203_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 52213_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 52213_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 20188_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 20188_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks
**** FOUND 10:02:41.12 +26:41:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29364_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160
The candidate 29364_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160 did not pass the final checks