This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR
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 27.2401* 10 39 57.16 +12 37 18.9 9.8 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
VARIABLE_NAME,2461098.7401,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.2401 9.79CV 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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:39:57.16 +12:37:18.9 ;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-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_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 27.2401* 10 50 16.02 +10 44 38.9 11.4 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,2461098.7401,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.2401 11.39CV 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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:50:16.02 +10:44:38.9 ;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-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_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 27.2401* 10 10 27.38 +13 47 11.6 11.9 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,2461098.7401,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.2401 11.86CV 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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:10:27.38 +13:47:11.6 ;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-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_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 27.2401* 10 33 32.61 +13 53 13.0 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,2461098.7401,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.2401 13.70CV 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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:33:32.61 +13:53:13.0 ;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-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_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 27.2401* 10 58 28.74 +11 37 00.6 14.3 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,2461098.7401,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.2401 14.31CV 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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:58:28.74 +11:37:00.6 ;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-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_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 27.2401* 10 43 28.45 +11 28 24.4 14.1 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,2461098.7401,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.2401 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:43:28.45 +11:28:24.4 ;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-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_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 27.2401* 10 21 30.94 +18 36 19.4 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
VARIABLE_NAME,2461098.7401,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.2401 13.84CV 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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:21:30.94 +18:36:19.4 ;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-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_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 27.2401* 10 31 30.30 +13 02 17.1 14.1 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,2461098.7401,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.2401 14.11CV 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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:31:30.30 +13:02:17.1 ;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-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20_00sec_-14_90C_LIGHT_0091_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: 2461058.87067979 18.01.2026 08:53:36.734 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
First image: 2461058.87067979 18.01.2026 08:53:36.734 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Last image: 2461098.74046980 27.02.2026 05:46:06.591 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 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): 6119
Objects passed selection criteria: 6109
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 5300.25
Average stars matched: 5199.25 (98.0944 %)
Memory usage VmPeak: 112476 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 Fri Feb 27 05:14:09 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: 2461058.87067979 18.01.2026 08:53:36.734 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
First image: 2461058.87067979 18.01.2026 08:53:36.734 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Last image: 2461098.74046980 27.02.2026 05:46:06.591 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 13 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 32531
Objects passed selection criteria: 32447
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 29070.8
Average stars matched: 27854 (95.8145 %)
Memory usage VmPeak: 135604 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 Fri Feb 27 05:15:09 CST 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR=
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE=
FRAME_EDGE_OFFSET_PIX= 100
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Leo-05-Q2b1x1
#######################################
########### Starting Leo-05-Q2b1x1 ###########
Processing Leo-05-Q2b1x1
server tau has sufficient free disk space available: 679544 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 679544 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.png' -> 'transient_report/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits_preview.png'
Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
renamed 'Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.png' -> 'transient_report/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits_preview.png'
Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 536.2055
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 493.8357
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1951.0258
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 593.4054
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1948.6860
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 595.7233
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 3.63858
INFO: SECOND_EPOCH__SD_ratio= 0.004
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
SExtractor catalog cache: saved Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat to cache
SExtractor catalog cache: saved Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.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: 2461098.73981647
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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits exists and is non-empty
Saving wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits to local_wcs_cache/
'wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits' -> 'local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits'
wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits exists and is non-empty
Saving wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits to local_wcs_cache/
'wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits' -> 'local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits'
wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits exists and is non-empty
Saving wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits to local_wcs_cache/
'wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits' -> 'local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits'
wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits exists and is non-empty
Saving wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits to local_wcs_cache/
'wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits' -> 'local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.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 10:40:00.041 +13:59:48.07
Second-epoch image center 10:39:46.770 +14:01:31.88
Angular distance between the image centers 0.06 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 10:40:00.041 +13:59:48.07
Second-epoch image center 10:39:44.847 +14:00:48.43
Angular distance between the image centers 0.06 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 10:39:46.770 +14:01:31.88
Second-epoch second image center 10:39:44.847 +14:00:48.43
Angular distance between the image centers 0.01436 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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits &> /tmp/tmp.xkqSBsJOp7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits &> /tmp/tmp.pDXP9Abw9K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits &> /tmp/tmp.Fp9PDz8YPw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits &> /tmp/tmp.eTJ6XGjJ2T
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
Found non-empty wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
The reference image (wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits) and catalog (wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat) found
'wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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 3596 out of 6443 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.884590
a=0.000000 b=1.000000 c=22.884590
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.35
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.35
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
2.1 pix Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
2.4 pix Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
2.4 pix Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
Limiting magnitude estimates:
15.4 mag. Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
15.4 mag. Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
14.6 mag. Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
14.6 mag. Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
All-image limiting magnitude estimate: 14.6 (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.xkqSBsJOp7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits' -> 'wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=439, passed=6443
Got 6443 stars (including 5991 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
util/solve_plate_with_UCAC5 got 6443 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 875 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: 0.25"
Excluding outliers - 875 stars left (next iteration limit 962)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits -region wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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.pDXP9Abw9K (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits' -> 'wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=445, passed=6432
Got 6432 stars (including 5975 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat
util/solve_plate_with_UCAC5 got 6432 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 871 stars left (next iteration limit 958)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits -region wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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.Fp9PDz8YPw (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_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.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_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=421, passed=4219
Got 4219 stars (including 3792 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat
util/solve_plate_with_UCAC5 got 4219 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 875 stars left (next iteration limit 962)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits -region wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.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.eTJ6XGjJ2T (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_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.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_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=426, passed=4241
Got 4241 stars (including 3814 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat
util/solve_plate_with_UCAC5 got 4241 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 876 stars left (next iteration limit 963)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits -region wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Leo-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20368.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 20348_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 20348_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 11:02:19.23 +16:30:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 2.145 3969885761146749824 165.58038003403 +16.50754342749 10.6395 9.6280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20355_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
Preparing report for the candidate 20355_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20368_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
Preparing report for the candidate 20368_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20387_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 20387_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:36:02.56 +13:32:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.409 3885494597287630336 159.01074133366 +13.54508740537 12.2761 11.7615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Leo-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:39:57.16 +12:37:18.9
10:50:16.02 +10:44:38.9
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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
SExtractor catalog cache: saved Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat to cache
SExtractor catalog cache: saved Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Creating symlink local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
Creating symlink local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
Creating symlink local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits exists and is non-empty
wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits exists and is non-empty
wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits exists and is non-empty
wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.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 10:40:00.041 +13:59:48.07
Second-epoch image center 10:39:46.770 +14:01:31.88
Angular distance between the image centers 0.06 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 10:40:00.041 +13:59:48.07
Second-epoch image center 10:39:44.847 +14:00:48.43
Angular distance between the image centers 0.06 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 10:39:46.770 +14:01:31.88
Second-epoch second image center 10:39:44.847 +14:00:48.43
Angular distance between the image centers 0.01436 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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits &> /tmp/tmp.Dx6fvUoHrb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits &> /tmp/tmp.3eu2LVFrRI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits &> /tmp/tmp.ReEQ77uqaH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits &> /tmp/tmp.eKUjHRoaZI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
Found non-empty wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
The reference image (wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits) and catalog (wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat) found
'wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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 3641 out of 34456 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.780203
a=0.000000 b=1.000000 c=22.780203
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
1.9 pix Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
2.2 pix Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
2.2 pix Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
Limiting magnitude estimates:
15.5 mag. Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
15.5 mag. Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
14.8 mag. Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
14.8 mag. Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.2 (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.Dx6fvUoHrb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits' -> 'wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1356, passed=34443
Got 34443 stars (including 33015 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
util/solve_plate_with_UCAC5 got 34443 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 875 stars left (next iteration limit 962)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits -region wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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.3eu2LVFrRI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits' -> 'wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1357, passed=34514
Got 34514 stars (including 33102 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat
util/solve_plate_with_UCAC5 got 34514 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 878 stars left (next iteration limit 965)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits -region wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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.ReEQ77uqaH (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_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.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_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=979, passed=24132
Got 24132 stars (including 23122 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat
util/solve_plate_with_UCAC5 got 24132 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 883 stars left (next iteration limit 971)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits -region wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-45-10_20.00sec_-14.90C_LIGHT_0091.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.eKUjHRoaZI (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_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.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_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat corresponding to the image wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=968, passed=24009
Got 24009 stars (including 23006 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat
util/solve_plate_with_UCAC5 got 24009 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 882 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: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 882 stars left (next iteration limit 970)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-05-Q2b1x1_050939_TTUQ2b1x1_25114_DNmeDSqR/Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits -region wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Leo-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53156.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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: 4s
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Considering the candidate 52288_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52288_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:21:14.80 +11:41:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.004 3883530255340092672 155.31150209520 +11.68293943945 14.4321 13.8982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52295_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52295_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 11:07:42.61 +16:56:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.860 3971386250920779776 166.92775614944 +16.94355749818 13.7521 13.1704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52299_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52299_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:57:55.98 +18:11:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.658 3983058460203415296 164.48339087917 +18.18759665379 13.3821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52300_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52300_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:30:03.52 +15:25:34.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 52301_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52301_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:47:37.21 +09:04:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.274 3869216091415236608 161.90518086266 +09.07979831432 12.7912 12.2916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52303_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52303_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 11:00:20.25 +13:11:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 0.589 3968032946614924672 165.08444871329 +13.18759152600 11.8510 11.1632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52309_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52309_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:39:57.16 +12:37:18.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52344_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52344_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:50:16.02 +10:44:38.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52396_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
Preparing report for the candidate 52396_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
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Considering the candidate 52600_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52600_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 11:08:39.20 +17:13:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.230 3971490528431907200 167.16338128710 +17.22251664208 12.8519 12.3609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52612_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52612_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:57:47.31 +15:37:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.691 3969359365659752832 164.44716814469 +15.63296517131 13.4625 12.8510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52684_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52684_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:48:08.01 +14:13:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.850 3885129838600264960 162.03386131497 +14.21823235245 13.8511 13.1986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52747_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52747_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:38:47.82 +16:07:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.322 3886459251237245312 159.69845389070 +16.12787760786 13.7097 13.2083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52749_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52749_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:42:06.36 +09:22:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.654 3869136101944504704 160.52631607480 +09.36883793585 14.0166 13.4840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52908_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
Preparing report for the candidate 52908_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
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Considering the candidate 52954_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 52954_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 11:10:20.91 +11:03:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.379 3964304640124348416 167.58727031053 +11.05239434184 13.7053 13.1526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52974_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
Preparing report for the candidate 52974_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
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Considering the candidate 53027_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
Preparing report for the candidate 53027_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
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Considering the candidate 53029_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 53029_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 10:31:36.76 +10:12:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.449 3882152807788897920 157.90357495901 +10.21636472685 14.2611 13.6845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53031_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
Preparing report for the candidate 53031_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
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Considering the candidate 53034_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 53034_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 11:09:39.21 +13:17:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 4.364 3965232387420132352 167.41330775042 +13.29140494084 14.2063 13.7117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53092_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092
The candidate 53092_Leo-05-Q2b1x1_2026-02-26_23-46-06_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
