This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa
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 22.2185* 10 33 37.60 +00 33 30.1 8.8 U Sex 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,2461093.7185,8.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2185 8.81CV 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:33:37.60 -00:33:30.1 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_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 22.2185* 10 42 00.71 -02 04 19.0 12.7 U Sex 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,2461093.7185,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2185 12.66CV 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:42:00.71 -02:04:19.0 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_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 22.2185* 09 58 44.94 +01 43 53.7 13.5 U Sex 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,2461093.7185,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2185 13.46CV 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:58:44.94 +01:43:53.7 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_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 22.2185* 09 47 39.49 +00 56 03.6 13.6 U Sex 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,2461093.7185,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2185 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:47:39.49 +00:56:03.6 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_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 22.2185* 10 24 15.06 -02 18 54.4 14.0 U Sex 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,2461093.7185,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2185 14.04CV 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:24:15.06 -02:18:54.4 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_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 22.2185* 10 30 41.18 +00 02 59.5 14.2 U Sex 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,2461093.7185,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2185 14.18CV 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:30:41.18 +00:02:59.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_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 22.2185* 10 45 27.07 -02 31 39.0 14.3 U Sex 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,2461093.7185,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2185 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:45:27.07 -02:31:39.0 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_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 22.2185* 10 12 01.13 -05 19 33.1 14.4 U Sex 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,2461093.7185,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2185 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:12:01.13 -05:19:33.1 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20_00sec_-15_00C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20_00sec_-15_00C_LIGHT_0201_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: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
First image: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Last image: 2461093.71867403 22.02.2026 05:14:43.436 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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: 4 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): 7619
Objects passed selection criteria: 7611
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 7235.25
Average stars matched: 7108 (98.2412 %)
Memory usage VmPeak: 113564 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 06:25:06 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: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
First image: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Last image: 2461093.71867403 22.02.2026 05:14:43.436 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 165
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 20 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): 41930
Objects passed selection criteria: 41840
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 40587
Average stars matched: 39096 (96.3264 %)
Memory usage VmPeak: 141956 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 06:26:35 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
SExtractor catalog cache: saved Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat to cache
SExtractor catalog cache: saved Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461093.71823494
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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits exists and is non-empty
Saving wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits to local_wcs_cache/
'wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'local_wcs_cache/wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits exists and is non-empty
Saving wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits to local_wcs_cache/
'wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'local_wcs_cache/wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits exists and is non-empty
Saving wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits to local_wcs_cache/
'wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits' -> 'local_wcs_cache/wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits'
wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
Saving wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits to local_wcs_cache/
'wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits' -> 'local_wcs_cache/wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.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 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:19.834 -01:59:10.12
Angular distance between the image centers 0.07 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 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:18.736 -01:59:04.16
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 10:17:19.834 -01:59:10.12
Second-epoch second image center 10:17:18.736 -01:59:04.16
Angular distance between the image centers 0.00486 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits &> /tmp/tmp.7ugA5kivwP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits &> /tmp/tmp.18nWtv5P7a
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits &> /tmp/tmp.NFFPV4enP3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.i2MjnOrshP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
Found non-empty wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
The reference image (wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits) and catalog (wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat) found
'wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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 4187 out of 7808 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.873666
a=0.000000 b=1.000000 c=22.873666
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
2.3 pix Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
2.2 pix fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
2.2 pix fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
Limiting magnitude estimates:
15.2 mag. Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
15.2 mag. Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
15.1 mag. fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
15.1 mag. fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.1 (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.7ugA5kivwP (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS-calibrated image found: wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Checking if the catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS catalog name: wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=466, passed=7808
Got 7808 stars (including 7337 good ones) from the SExtractor catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
util/solve_plate_with_UCAC5 got 7808 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 931 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 931 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: 0.28"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits -region wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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.18nWtv5P7a (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS-calibrated image found: wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Checking if the catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS catalog name: wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=461, passed=7862
Got 7862 stars (including 7394 good ones) from the SExtractor catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
util/solve_plate_with_UCAC5 got 7862 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 934 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 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits -region wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.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.NFFPV4enP3 (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_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.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_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
Checking if the catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
WCS catalog name: wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=513, passed=6799
Got 6799 stars (including 6274 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 6799 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 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 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 - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits -region wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.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.i2MjnOrshP (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_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.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_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=526, passed=6761
Got 6761 stars (including 6227 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 6761 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 935 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits'
Saving fully-calibrated image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits'
Preparing the HTML report for the field Sex-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20394.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20394_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
Preparing report for the candidate 20394_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20422_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 20422_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:57:22.32 -02:32:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 2.295 3829542649573111808 149.34236551713 -02.54873683231 11.1063 9.6145 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20424_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 20424_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:18:47.16 -00:26:06.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Sex-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:33:37.60 -00:33:30.1
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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
SExtractor catalog cache: saved Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat to cache
SExtractor catalog cache: saved Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Creating symlink local_wcs_cache/wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Creating symlink local_wcs_cache/wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
Creating symlink local_wcs_cache/wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits exists and is non-empty
wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits exists and is non-empty
wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits exists and is non-empty
wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.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 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:19.834 -01:59:10.12
Angular distance between the image centers 0.07 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 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:18.736 -01:59:04.16
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 10:17:19.834 -01:59:10.12
Second-epoch second image center 10:17:18.736 -01:59:04.16
Angular distance between the image centers 0.00486 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits &> /tmp/tmp.Ti2WDmjasr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits &> /tmp/tmp.BmRm6tURLM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits &> /tmp/tmp.3W9z3zApsG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.3Ndpr2gx4D
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
Found non-empty wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
The reference image (wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits) and catalog (wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat) found
'wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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 4239 out of 40923 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.755742
a=0.000000 b=1.000000 c=22.755742
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 81 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
2.3 pix Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
2.0 pix fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
2.0 pix fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
Limiting magnitude estimates:
15.3 mag. Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
15.3 mag. Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
15.2 mag. fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
15.2 mag. fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Ti2WDmjasr (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS-calibrated image found: wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Checking if the catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS catalog name: wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1914, passed=40911
Got 40911 stars (including 38933 good ones) from the SExtractor catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
util/solve_plate_with_UCAC5 got 40911 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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits -region wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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.BmRm6tURLM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS-calibrated image found: wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Checking if the catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS catalog name: wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1902, passed=40634
Got 40634 stars (including 38663 good ones) from the SExtractor catalog wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
util/solve_plate_with_UCAC5 got 40634 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 931 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: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits -region wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.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.3W9z3zApsG (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_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.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_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
Checking if the catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
WCS catalog name: wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1835, passed=41001
Got 41001 stars (including 39089 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 41001 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 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits -region wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.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.3Ndpr2gx4D (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_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.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_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1891, passed=41152
Got 41152 stars (including 39181 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 41152 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 930 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-05_20.00sec_-15.00C_LIGHT_0201.fits
Saving fully-calibrated image wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Sex-02-Q1b1x1_231621_TTUQ1b1x1_11110_AxTkHpxa/wcs_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202.fits
Preparing the HTML report for the field Sex-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52869.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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 52628_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52628_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:56:57.44 -06:58:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 3.686 3821313599608680064 149.23955465770 -06.96930538815 14.6816 13.9495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52633_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52633_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:57:23.77 -04:49:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 0.230 3822239010442053888 149.34903602542 -04.82356358147 14.8429 14.3245 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52638_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52638_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:13:02.59 -05:31:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52643_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52643_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:59:14.43 -06:01:34.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52644_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52644_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:54:12.23 -01:01:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52645_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52645_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:56:58.79 -05:08:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.006 3821842499061331840 149.24510455523 -05.14737272299 14.1701 13.6955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.006#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52648_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52648_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:17:42.03 -04:43:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.461 3779837169150539648 154.42488425986 -04.72770034797 14.0309 13.5537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52650_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52650_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:07:31.86 -06:37:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.019 3773488279774239360 151.88327475180 -06.62476268055 13.8657 13.2423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52651_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52651_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:29:56.40 -06:55:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.001 3775713893171721856 157.48526899542 -06.91814441231 13.7417 13.1600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52652_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52652_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:49:05.82 -04:41:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52653_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52653_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:59:13.46 -02:18:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52655_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52655_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:15:42.35 -06:27:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52656_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52656_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:30:09.77 -03:51:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.172 3780892214981309440 157.54038212387 -03.86287219490 12.9326 12.4493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52657_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52657_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:10:16.69 -01:55:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.252 3829042650955575168 152.56978229623 -01.92861234397 12.7713 12.2415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52658_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52658_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:41:25.55 -02:06:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.392 3805555983074750208 160.35678534630 -02.11593222841 12.8438 12.2566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52659_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52659_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:57:43.18 +01:55:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52660_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52660_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:56:43.16 -04:04:06.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52661_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52661_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:03:11.52 -06:57:34.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52664_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52664_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:33:37.59 -00:33:30.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52684_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52684_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:55:45.41 -04:55:02.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52694_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52694_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:08:28.91 -03:29:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52702_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
Preparing report for the candidate 52702_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52708_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52708_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52718_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52718_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 52722_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52722_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52725_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52725_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52726_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52726_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52736_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52736_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:02:22.32 -04:46:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52746_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52746_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:56:08.38 +01:26:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52747_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
Preparing report for the candidate 52747_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52749_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52749_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52752_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52752_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:49:08.77 -06:17:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52755_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52755_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:54:07.36 -03:32:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52756_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52756_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:57:20.33 +01:12:29.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52760_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
Preparing report for the candidate 52760_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52766_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52766_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:22:53.52 -06:36:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.513 3775643597442573056 155.72306150745 -06.60239894136 13.7229 13.0628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52767_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52767_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:11:40.84 +02:12:34.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52768_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52768_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:16:45.98 -03:07:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52770_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52770_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:25:43.85 +01:28:08.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52773_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52773_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:10:19.19 -05:01:31.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52774_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52774_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:18:18.79 -01:13:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.471 3830639519796391680 154.57840493548 -01.22693442630 13.8072 13.3324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52776_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52776_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:59:32.52 -01:10:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52777_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52777_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:49:41.88 -03:40:53.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52778_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52778_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52781_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52781_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:12:14.14 -03:47:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52787_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52787_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:12:43.82 +02:12:15.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52802_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
Preparing report for the candidate 52802_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52804_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52804_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:44:50.37 +03:00:31.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52805_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52805_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:00:23.89 +00:03:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52806_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52806_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:02:19.02 -05:46:40.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52809_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52809_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52815_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52815_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:57:12.28 -04:12:36.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52820_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52820_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:34:03.42 +02:48:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 2.791 3856141759994584064 158.51489165890 +02.80711953541 14.3285 13.8469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52823_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52823_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52826_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52826_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:12:46.03 -07:00:20.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52827_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
Preparing report for the candidate 52827_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52829_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52829_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:57:16.48 +00:56:52.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52834_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52834_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:49:53.04 -04:15:40.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52837_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52837_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:02:24.71 -02:56:47.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52838_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
Preparing report for the candidate 52838_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52840_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52840_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52844_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52844_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52847_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52847_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52849_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52849_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:05:33.89 -04:59:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52858_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52858_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:15:14.58 +01:02:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52859_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52859_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52862_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52862_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:01:44.05 +01:07:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 3.102 3833688529964774784 150.43439141227 +01.13317095401 14.5185 13.7912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52865_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52865_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:21:17.83 -05:42:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52869_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
Preparing report for the candidate 52869_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
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Considering the candidate 52870_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52870_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52878_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52878_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52879_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52879_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:46:56.79 -01:54:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 2.437 3827535186154312576 146.73728423122 -01.91018282830 14.5078 14.0131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52885_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52885_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:09:46.52 +01:06:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.576 3835035607802394880 152.44411976241 +01.09972453855 14.3438 13.6789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52886_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52886_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:04:54.36 -03:45:33.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)
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Considering the candidate 52894_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52894_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:06:12.23 -04:44:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 2.840 3822069715716190208 151.55173605539 -04.74139639266 14.7100 14.1915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52900_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52900_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:49:29.26 +00:17:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.349 3834134661102655872 147.37183178486 +00.29929698266 14.6769 14.1391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52905_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52905_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:04:12.44 -01:34:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.156 3830048360497676288 151.05225075557 -01.57112608969 14.1952 13.2316 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52926_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52926_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:59:17.63 +02:33:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 1.022 3836331760212736768 149.82373303245 +02.55870531971 14.4695 13.9423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52934_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52934_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:09:25.27 -06:23:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52935_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52935_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 09:49:38.67 -03:24:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52947_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202
The candidate 52947_fd_Sex-02-Q1b1x1_2026-02-21_23-14-43_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks