This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.8949,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.3949 11.05CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:28:27.64 -26:56:45.7 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
UY Sco,2461098.8949,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UY Sco 20260227.3949 11.22CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:14:40.30 -21:42:06.7 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CI Sco,2461098.8949,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CI Sco 20260227.3949 11.61CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:42:01.42 -29:45:07.6 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SSS_J162642.0-295716,2461098.8949,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SSS_J162642.0-295716 20260227.3949 12.13CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:26:41.99 -29:57:18.5 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.8949,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260227.3949 12.94CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:51:36.45 -23:53:07.5 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.8949,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.3949 13.10CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:39:39.24 -22:22:22.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
UZ Sco,2461098.8949,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UZ Sco 20260227.3949 11.38CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:15:40.24 -25:01:02.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SSS_J160319.9-233220,2461098.8949,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SSS_J160319.9-233220 20260227.3949 12.62CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:03:19.75 -23:32:21.7 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GL Sco,2461098.8949,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GL Sco 20260227.3949 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:06:49.11 -22:38:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J160733-2941.3,2461098.8949,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J160733-2941.3 20260227.3949 10.62CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:07:33.32 -29:41:17.4 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1328 Sco,2461098.8949,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1328 Sco 20260227.3949 12.51CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:03:31.85 -28:12:07.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GU Sco,2461098.8949,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GU Sco 20260227.3949 11.62CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:50:23.72 -28:11:35.0 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TZ Sco,2461098.8949,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TZ Sco 20260227.3949 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:07:42.86 -23:18:55.7 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RX Sco,2461098.8949,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RX Sco 20260227.3949 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:11:57.29 -24:53:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J161520-2919.6,2461098.8949,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J161520-2919.6 20260227.3949 12.18CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:15:20.41 -29:19:29.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J162405-2815.2,2461098.8949,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J162405-2815.2 20260227.3949 9.76CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:24:05.29 -28:15:13.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J161722-2455.5,2461098.8949,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J161722-2455.5 20260227.3949 10.90CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:17:22.04 -24:55:32.0 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461059.00651774 18.01.2026 12:09:13.133 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461059.00651774 18.01.2026 12:09:13.133 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461098.89518164 27.02.2026 09:28:53.694 /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 25
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.43
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5577
Objects passed selection criteria: 5572
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 4929.5
Average stars matched: 4816.5 (97.7077 %)
Memory usage VmPeak: 112012 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 Mar 1 06:53:03 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461059.00651774 18.01.2026 12:09:13.133 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461059.00651774 18.01.2026 12:09:13.133 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461098.89518164 27.02.2026 09:28:53.694 /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 77
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.16
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 13 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 49807
Objects passed selection criteria: 49769
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 45364.8
Average stars matched: 43778.5 (96.5033 %)
Memory usage VmPeak: 152352 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 Mar 1 06:54:07 CST 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR=
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE=
FRAME_EDGE_OFFSET_PIX= 100
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Sco-02-Q2b1x1
#######################################
########### Starting Sco-02-Q2b1x1 ###########
Processing Sco-02-Q2b1x1
server tau has sufficient free disk space available: 642451 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 642451 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.png' -> 'transient_report/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits_preview.png'
Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
renamed 'Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.png' -> 'transient_report/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits_preview.png'
Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 2896.5301
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 833.1114
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 5518.8426
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 1522.4618
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 5485.4272
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 1511.4552
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.90533
INFO: SECOND_EPOCH__SD_ratio= 0.007
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461098.89460579
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits'
wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits'
wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits'
wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits'
The image scale is 5.92"/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 16:19:25.170 -25:57:36.18
Second-epoch image center 16:19:12.224 -26:00:19.00
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 16:19:25.170 -25:57:36.18
Second-epoch image center 16:19:14.979 -26:00:11.22
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 16:19:12.224 -26:00:19.00
Second-epoch second image center 16:19:14.979 -26:00:11.22
Angular distance between the image centers 0.01054 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.00GMP1gBFO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits &> /tmp/tmp.ejI6C40cBO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits &> /tmp/tmp.qGT3FwcopM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits &> /tmp/tmp.6sA9dczPWY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.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 4489 out of 5898 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.565703
a=0.000000 b=1.000000 c=22.565703
From vast_summary.log: estimated ref. image limiting mag.: -8.43
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.14
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.14
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 24 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
2.3 pix Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
2.6 pix Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
2.6 pix Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
Limiting magnitude estimates:
14.1 mag. Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
14.1 mag. Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
13.6 mag. Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
13.6 mag. Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 10.9 (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.00GMP1gBFO (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=416, passed=5898
Got 5898 stars (including 5474 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 5898 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.2'
Seting catalog search parameters based on the expected field of view 944.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013114 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010491 (37.8 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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.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.ejI6C40cBO (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits' -> 'wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=413, passed=5849
Got 5849 stars (including 5431 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat
util/solve_plate_with_UCAC5 got 5849 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.0'
Seting catalog search parameters based on the expected field of view 944.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013111 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010489 (37.8 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 960 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: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits -region wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.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.qGT3FwcopM (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=385, passed=4043
Got 4043 stars (including 3658 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat
util/solve_plate_with_UCAC5 got 4043 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.0'
Seting catalog search parameters based on the expected field of view 940.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013056 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010444 (37.6 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 969 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: 0.83"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.82"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.81"
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.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.6sA9dczPWY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=397, passed=4033
Got 4033 stars (including 3633 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat
util/solve_plate_with_UCAC5 got 4033 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.9'
Seting catalog search parameters based on the expected field of view 939.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013054 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010443 (37.6 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 968 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out01082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20395.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 20368_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20368_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:06:49.10 -22:38:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20369_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20369_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:11:57.29 -24:53:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.20, MAG_FAINT_SEARCH_LIMIT=11.18)GAIADR2_OUTPUT=# 0.519 6049589774341204480 242.98867590796 -24.89894218214 10.3565 8.9075 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20373_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20373_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:17:22.04 -24:55:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 0.131 6049636228705353728 244.34180785156 -24.92544399157 9.9566 8.5315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20374_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20374_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:16:47.46 -23:11:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 1.634 6050365823392459008 244.19725840817 -23.19476266583 10.1197 8.8751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20375_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20375_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:22:18.01 -25:12:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 0.835 6048992258488336896 245.57515428951 -25.21434720587 10.9170 10.1721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20376_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20376_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:19:35.45 -26:29:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 0.487 6048395498552642432 244.89775207707 -26.48378719767 10.9416 10.1786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20379_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 20379_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20380_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20380_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:29:45.54 -29:45:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 3.147 6043838469539432960 247.44052389102 -29.75855938322 9.4869 7.9765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20381_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20381_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:19:14.18 -25:34:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 0.182 6048771531528673792 244.80912232625 -25.57306408323 10.7613 9.7155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20382_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20382_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:11:48.55 -25:49:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.08, MAG_FAINT_SEARCH_LIMIT=12.06)GAIADR2_OUTPUT=# 0.263 6043471954204730496 242.95223089434 -25.81938170801 11.1835 10.6382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20383_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20383_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:23:36.91 -25:46:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 1.055 6048539534578287360 245.90379316768 -25.77851243115 10.5678 9.4096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20386_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20386_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:24:13.73 -25:12:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 0.221 6049004009519228416 246.05727593679 -25.21280953926 11.0531 10.3167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20387_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20387_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:12:15.14 -25:43:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 0.625 6049478895464571392 243.06300497111 -25.71892473961 10.3093 9.0208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20388_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20388_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:18:36.19 -27:51:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 0.296 6039293225902481536 244.65072874075 -27.86480053204 11.0319 10.3262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20390_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20390_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:12:21.28 -25:32:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 0.112 6049485625671832448 243.08869347663 -25.53550800169 11.1093 10.3702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20391_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20391_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:11:23.37 -27:27:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 0.567 6042463427164518656 242.84735468638 -27.45939910254 10.9915 10.1426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20392_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20392_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:03:57.76 -25:59:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 0.232 6043630146447240064 240.99073801483 -25.99789497028 11.4310 11.1116 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20393_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20393_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:14:43.10 -28:29:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 1.139 6039145685186131584 243.67974577633 -28.48831013786 10.4018 9.1753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20394_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20394_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:07:18.33 -25:55:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 0.108 6043596370823705216 241.82639561227 -25.93249567394 11.1392 10.3745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20395_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 20395_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20397_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20397_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:07:59.08 -29:23:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 0.595 6041633089736435072 241.99598548265 -29.39056170510 10.1375 8.7896 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20399_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20399_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:09:16.56 -26:10:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 0.379 6043481089596450944 242.31910739376 -26.17229208319 11.2628 10.7773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20412_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 20412_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:01:00.38 -27:35:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 0.307 6042833309753276288 240.25151686872 -27.59907712122 10.9591 10.0994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01082_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 01082_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:07:33.31 -29:41:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)GAIADR2_OUTPUT=# 1.411 6041587391283378944 241.88859900331 -29.68854895513 9.4722 8.0108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:28:27.64 -26:56:45.7
16:14:40.30 -21:42:06.7
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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits exists and is non-empty
wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits exists and is non-empty
wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits exists and is non-empty
The image scale is 5.92"/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 16:19:25.170 -25:57:36.18
Second-epoch image center 16:19:12.224 -26:00:19.00
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 16:19:25.170 -25:57:36.18
Second-epoch image center 16:19:14.979 -26:00:11.22
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 16:19:12.224 -26:00:19.00
Second-epoch second image center 16:19:14.979 -26:00:11.22
Angular distance between the image centers 0.01054 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.S8AwDD3A4u
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits &> /tmp/tmp.RpwNzooyFC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits &> /tmp/tmp.gVh3h2hWQo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits &> /tmp/tmp.IUVutdVnnl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.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 6883 out of 55971 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.333637
a=0.000000 b=1.000000 c=22.333637
From vast_summary.log: estimated ref. image limiting mag.: -8.16
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.17
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 68 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
2.3 pix Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
2.5 pix Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
2.5 pix Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
Limiting magnitude estimates:
14.2 mag. Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
14.1 mag. Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
13.7 mag. Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
13.8 mag. Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.S8AwDD3A4u (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=2488, passed=55966
Got 55966 stars (including 53372 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 55966 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.2'
Seting catalog search parameters based on the expected field of view 944.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013114 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010491 (37.8 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 965 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.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.RpwNzooyFC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits' -> 'wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2480, passed=53562
Got 53562 stars (including 50994 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat
util/solve_plate_with_UCAC5 got 53562 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.0'
Seting catalog search parameters based on the expected field of view 944.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013111 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010489 (37.8 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 967 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits -region wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.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.gVh3h2hWQo (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1481, passed=36120
Got 36120 stars (including 34594 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat
util/solve_plate_with_UCAC5 got 36120 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.0'
Seting catalog search parameters based on the expected field of view 940.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013056 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010444 (37.6 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 975 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: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.76"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.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.IUVutdVnnl (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1505, passed=37318
Got 37318 stars (including 35765 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat
util/solve_plate_with_UCAC5 got 37318 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.9'
Seting catalog search parameters based on the expected field of view 939.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013054 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010443 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out12723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21934.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71097.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out67923.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out08346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71055.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 7s
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Considering the candidate 70668_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70668_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:17:04.42 -23:40:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.460 6050315864332202240 244.26840036377 -23.66751127561 13.5097 12.6207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70669_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70669_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:51:47.68 -21:06:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 3.922 4127111006181290112 252.94773509142 -21.10754588954 11.7188 11.0738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70671_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70671_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:52:06.09 -28:55:40.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)
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Considering the candidate 70672_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70672_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:52:54.15 -30:45:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.746 6027984577058799104 253.22475841074 -30.75308115278 10.8757 10.6590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70674_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70674_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:51:30.37 -21:04:38.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 70675_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70675_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:00:13.30 -24:18:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.267 6236195486194570752 240.05536054267 -24.30306859058 12.8746 11.8671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70682_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70682_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 70683_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70683_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:33:58.99 -26:01:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 1.047 6045703481774542976 248.49550707423 -26.03227786386 12.4375 11.7778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70712_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70712_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:28:27.63 -26:56:45.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 70734_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70734_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:21:00.14 -25:36:03.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 70754_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 70754_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
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Considering the candidate 70767_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70767_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:02:33.33 -26:10:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 1.017 6043249681062336384 240.63918722208 -26.17206301919 12.0177 11.4699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70804_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 70804_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
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Considering the candidate 70810_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70810_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:23:16.38 -29:56:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.810 6037970234235703552 245.81844418978 -29.93426049496 12.7510 10.6858 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70870_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70870_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:13:51.10 -24:25:39.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 70889_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70889_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:49:30.25 -22:37:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70910_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70910_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:32:40.29 -29:39:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.349 6031853376174239488 248.16780350612 -29.65667742773 11.7085 10.3606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70944_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 70944_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70950_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70950_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:11:43.86 -22:09:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.139 6242875397286763136 242.93265062175 -22.15724724642 13.3413 12.7694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70952_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70952_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:09:34.78 -27:53:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.075 6042052175461953152 242.39428954867 -27.89504697232 12.9877 12.1819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70955_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70955_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:02:15.19 -25:55:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.583 6043643340586741120 240.56372673595 -25.91703372776 13.2119 12.6794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70957_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70957_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:15:37.07 -29:50:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 0.402 6038452340034201600 243.90433388979 -29.84574953592 12.3129 10.9898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70958_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70958_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 15:54:24.62 -30:24:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.443 6040603328370438016 238.60247130942 -30.41172926733 12.4921 11.9815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70973_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70973_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 15:48:50.18 -27:11:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.160 6233886404393329792 237.21000634197 -27.19336651099 12.7312 11.8113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70984_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70984_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:13:35.68 -21:24:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.027 6243031596656446592 243.39823752825 -21.41681351125 13.1955 12.5434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70996_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 70996_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:26:30.57 -29:07:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.139 6044129805757064960 246.62715811172 -29.12482997386 13.3720 11.5004 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71010_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71010_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 15:50:35.86 -23:14:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 0.194 6240300749071319808 237.64946385646 -23.24980150780 12.5576 11.6540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71014_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71014_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 15:48:21.99 -26:30:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.464 6234063120830441088 237.09227407659 -26.51623942456 12.8982 12.3666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71017_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71017_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:05:42.72 -21:49:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.088 6243323650133943680 241.42808325237 -21.82343011947 12.9130 12.1137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71030_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71030_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:39:03.19 -27:01:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 2.485 6044650076619328256 249.76395933988 -27.01942742557 11.8835 10.5019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71055_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 71055_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71060_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71060_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:18:05.40 -21:49:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.323 6244258681693675648 244.52286806441 -21.81780174427 10.8833 9.9334 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71083_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71083_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:44:38.22 -29:16:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.733 6031399969397725568 251.16041562680 -29.27212033372 13.5864 12.0143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71097_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71097_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:43:10.22 -25:19:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.510 6046550307583907456 250.79365586669 -25.32658923259 11.8931 10.4310 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71102_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71102_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:24:04.79 -25:34:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.612 6048918896147458944 246.01967388470 -25.57029964451 12.1630 10.6961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71115_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71115_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:17:03.89 -26:41:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.105 6048412639764624512 244.26639627109 -26.69802069719 12.4238 11.0166 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71156_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71156_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:29:29.20 -22:49:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 1.539 6051040403835047552 247.37147761908 -22.83344579160 11.8287 10.3258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71180_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71180_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:08:48.81 -24:20:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.754 6049846956982747520 242.20389879783 -24.34062411074 13.9261 13.2086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71204_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71204_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:04:07.69 -27:00:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.192 6042969717916278912 241.03198861832 -27.01138587285 13.8168 13.0018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71210_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71210_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:02:45.25 -23:13:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.379 6242366082891663744 240.68838216737 -23.23285400826 13.8205 13.1957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71211_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71211_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:07:12.49 -25:45:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.939 6043696048419053056 241.80214939788 -25.76401979044 13.6987 13.1445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71219_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71219_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:04:10.65 -26:10:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 0.984 6043574414950470784 241.04418587310 -26.17526985243 13.7288 12.9974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71247_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71247_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 15:56:12.94 -25:25:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.186 6235688954929344768 239.05419937097 -25.43212502097 13.5946 13.0829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71256_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71256_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:19:22.17 -21:15:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.557 6244302288501965952 244.84280445122 -21.25446971371 13.6856 12.9146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71278_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71278_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:15:45.89 -23:35:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.098 6050332116488375552 243.94173544117 -23.58752056066 13.9469 13.2951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71288_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71288_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 15:53:43.88 -27:07:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.244 6233794560815995648 238.43313934177 -27.12245419979 13.3807 12.6002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71294_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71294_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:12:40.24 -23:29:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.239 6050019889546822144 243.16803436367 -23.49873597972 13.7857 12.9757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71312_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71312_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:21:36.03 -23:16:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 0.857 6050269650480022784 245.40034772307 -23.27923948181 13.5523 12.4207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71317_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 71317_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:18:43.85 -23:12:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.840 6050447118530640512 244.68188331149 -23.20755087080 13.9799 13.3239 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 66721_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 66721_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:38:12.81 -28:34:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 3.588 6032396951545882496 249.55449205471 -28.56939868827 10.5259 8.9585 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 36692_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 36692_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
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Considering the candidate 67157_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 67157_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:36:58.22 -29:44:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 3.241 6031691168165742080 249.24355828387 -29.73563957053 12.7630 10.3764 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51302_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 51302_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
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Considering the candidate 45698_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 45698_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
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Considering the candidate 66649_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 66649_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:23:53.57 -26:30:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.569 6045465574954001152 245.97323841529 -26.50157227284 13.0075 12.3771 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 46942_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 46942_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:14:40.30 -21:42:06.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 08346_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 08346_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
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Considering the candidate 17340_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 17340_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
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Considering the candidate 17626_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 17626_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
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Considering the candidate 12723_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 12723_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:32:18.78 -29:06:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.861 6043977832637073280 248.07797861431 -29.10567043502 11.9945 10.7445 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 49577_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 49577_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
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Considering the candidate 37115_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
Preparing report for the candidate 37115_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
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Considering the candidate 67923_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 67923_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 15:57:34.01 -30:08:27.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)
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Considering the candidate 21934_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 21934_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
**** FOUND 16:25:53.10 -27:34:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 0.872 6045167847812290816 246.47127019945 -27.58300832092 11.0595 9.5679 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67671_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185
The candidate 67671_Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185 did not pass the final checks
