This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.2289* 10 28 37.09 +00 06 03.7 8.7 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7289,8.66,0.05,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 20260227.2289 8.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:28:37.09 -00:06:03.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.2289* 10 37 08.20 -01 35 23.2 12.5 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7289,12.53,0.05,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 20260227.2289 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:37:08.20 -01:35:23.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.2289* 10 20 28.82 -01 50 23.8 13.7 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7289,13.71,0.05,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 20260227.2289 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:20:28.82 -01:50:23.8 ;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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.2289* 10 27 03.45 +00 42 54.0 13.9 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7289,13.89,0.05,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 20260227.2289 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:27:03.45 +00:42:54.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.2289* 10 41 02.41 -01 50 01.1 14.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7289,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.2289 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:41:02.41 -01:50:01.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.2289* 10 08 04.94 -04 36 43.5 14.3 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7289,14.26,0.05,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 20260227.2289 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:08:04.94 -04:36:43.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.2289* 09 54 08.27 +02 00 28.9 14.0 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7289,14.03,0.05,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 20260227.2289 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:54:08.27 +02:00:28.9 ;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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20_00sec_-14_90C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20_00sec_-15_00C_LIGHT_0072_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
First image: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Last image: 2461098.72913382 27.02.2026 05:29:47.162 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 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): 7452
Objects passed selection criteria: 7435
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 6312
Average stars matched: 6204.5 (98.2969 %)
Memory usage VmPeak: 113564 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Feb 27 06:48:46 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
First image: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Last image: 2461098.72913382 27.02.2026 05:29:47.162 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 42
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 17 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): 38375
Objects passed selection criteria: 38307
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 35146.2
Average stars matched: 33877 (96.3887 %)
Memory usage VmPeak: 140676 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Feb 27 06:49:46 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:
Sex-02-Q2b1x1
#######################################
########### Starting Sex-02-Q2b1x1 ###########
Processing Sex-02-Q2b1x1
server tau has sufficient free disk space available: 655229 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 655229 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.png' -> 'transient_report/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits_preview.png'
Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
renamed 'Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.png' -> 'transient_report/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits_preview.png'
Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.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= 661.1196
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 490.0839
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 2228.5049
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 629.2280
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 2227.1381
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 629.0010
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 3.3708
INFO: SECOND_EPOCH__SD_ratio= 0.000
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat to cache
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.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: 2461098.72859707
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits exists and is non-empty
Saving wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits to local_wcs_cache/
'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits exists and is non-empty
Saving wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits to local_wcs_cache/
'wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits exists and is non-empty
Saving wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits to local_wcs_cache/
'wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits' -> 'local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits'
wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits exists and is non-empty
Saving wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits to local_wcs_cache/
'wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits' -> 'local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:17.699 -01:59:35.62
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:15.025 -01:59:35.80
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:17:17.699 -01:59:35.62
Second-epoch second image center 10:17:15.025 -01:59:35.80
Angular distance between the image centers 0.01114 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits &> /tmp/tmp.tkZNzIitFL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits &> /tmp/tmp.XWKeS9bE5R
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits &> /tmp/tmp.xp5fW3D8k2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits &> /tmp/tmp.3bNbArRY3H
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
The reference image (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits) and catalog (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat) found
'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 4187 out of 7808 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.873666
a=0.000000 b=1.000000 c=22.873666
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
2.4 pix Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
2.4 pix Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
Limiting magnitude estimates:
15.2 mag. Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
15.2 mag. Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
14.6 mag. Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
14.6 mag. Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.7 (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.tkZNzIitFL (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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=466, passed=7808
Got 7808 stars (including 7337 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
util/solve_plate_with_UCAC5 got 7808 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.XWKeS9bE5R (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/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=461, passed=7862
Got 7862 stars (including 7394 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
util/solve_plate_with_UCAC5 got 7862 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xp5fW3D8k2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=507, passed=4880
Got 4880 stars (including 4368 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat
util/solve_plate_with_UCAC5 got 4880 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits -region wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.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.3bNbArRY3H (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=510, passed=4910
Got 4910 stars (including 4397 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat
util/solve_plate_with_UCAC5 got 4910 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits -region wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.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 Sex-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20421.dat to exclusion_list_gaiadr2.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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20395_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
Preparing report for the candidate 20395_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20409_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 20409_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 09:55:45.40 -04:55:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 1.806 3821864386214627712 148.93963379440 -04.91754824178 11.6457 10.9846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20421_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 20421_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:18:47.14 -00:26:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.235 3830845880089812736 154.69644542319 -00.43550301644 12.3223 11.7387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.235#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: 6s
Prepared the HTML report for the field Sex-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 ####
10:28:37.09 -00:06:03.7
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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat to cache
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Creating symlink local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Creating symlink local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
Creating symlink local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits exists and is non-empty
wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits exists and is non-empty
wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits exists and is non-empty
wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:17.699 -01:59:35.62
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:15.025 -01:59:35.80
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:17:17.699 -01:59:35.62
Second-epoch second image center 10:17:15.025 -01:59:35.80
Angular distance between the image centers 0.01114 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits &> /tmp/tmp.h1XJNJCJ89
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits &> /tmp/tmp.xD1TXzLISR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits &> /tmp/tmp.bwq3aIJml6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits &> /tmp/tmp.5XOZUReP2O
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
The reference image (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits) and catalog (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat) found
'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 4239 out of 40923 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.755742
a=0.000000 b=1.000000 c=22.755742
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 36 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
2.2 pix Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
2.2 pix Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
Limiting magnitude estimates:
15.3 mag. Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
15.3 mag. Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
14.8 mag. Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
14.7 mag. Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (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.h1XJNJCJ89 (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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1914, passed=40911
Got 40911 stars (including 38933 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
util/solve_plate_with_UCAC5 got 40911 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xD1TXzLISR (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/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1902, passed=40634
Got 40634 stars (including 38663 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
util/solve_plate_with_UCAC5 got 40634 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bwq3aIJml6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1367, passed=30155
Got 30155 stars (including 28751 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat
util/solve_plate_with_UCAC5 got 30155 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits -region wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-00_20.00sec_-15.00C_LIGHT_0072.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.5XOZUReP2O (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1414, passed=30106
Got 30106 stars (including 28646 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat
util/solve_plate_with_UCAC5 got 30106 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Sex-02-Q2b1x1_055754_TTUQ2b1x1_16246_tIoDyZgo/Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits -region wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073.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 Sex-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53548.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52603_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52603_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:47:31.66 -06:33:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 3.848 3764365043387545984 161.88096402275 -06.56558636389 13.2740 12.8274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52605_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52605_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:24:27.00 -03:52:07.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52607_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52607_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:13:34.50 -02:54:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.039 3828683385531284096 153.39403185893 -02.91478561499 14.9191 14.4855 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52608_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52608_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:03:53.72 -05:34:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 0.558 3773866683572788608 150.97367846923 -05.58204314958 13.9932 13.4738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52609_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52609_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 09:49:05.88 -04:41:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52618_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52618_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 09:55:11.86 -00:53:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 5.608 3833008000986000640 148.80074840260 -00.89896956746 14.4110 13.8408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52619_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52619_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:13:02.64 -05:31:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.749 3779677563870256128 153.26086820007 -05.52266158766 14.2182 13.6984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52621_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52621_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:20:15.29 -05:44:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.129 3778765110953721344 155.06367282868 -05.74810559974 14.2443 13.7768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52622_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52622_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:31:06.05 -03:16:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 1.363 3781206782681639680 157.77545748854 -03.27235344907 14.1689 13.6808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52624_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52624_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:43:30.18 -03:20:45.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)
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Considering the candidate 52625_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52625_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 09:58:30.09 +01:40:32.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
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Considering the candidate 52627_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52627_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:35:12.88 -00:14:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.501 3806795059664257792 158.80371330006 -00.24398007327 13.6587 13.1637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52629_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52629_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 09:57:07.59 +01:48:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.053 3834730940002150400 149.28199607161 +01.81587629780 12.9419 12.3470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52633_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52633_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 09:56:43.13 -04:04:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 2.320 3823101061918092416 149.18001333226 -04.06826524016 12.7090 12.1893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52637_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52637_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:28:37.10 -00:06:03.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52759_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52759_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:13:44.17 -05:12:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.575 3779760615653425792 153.43393283392 -05.20341060318 12.5911 12.1084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52783_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
Preparing report for the candidate 52783_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
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Considering the candidate 52816_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52816_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:27:13.35 -04:56:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 0.913 3779252263324343808 156.80546832488 -04.94895003572 13.1877 12.4727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52865_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52865_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:34:35.90 +01:46:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.838 3855728240543545856 158.64976843933 +01.77639125304 12.7654 12.3280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52967_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52967_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:32:05.19 -05:48:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.019 3775969289107226240 158.02189139363 -05.81242824425 13.3926 12.8872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52984_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52984_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:16:45.99 -03:07:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.690 3780707501323370752 154.19181073183 -03.12192414656 13.8418 13.3375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52990_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 52990_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:26:49.68 -00:07:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.332 3831047713488040704 156.70696481022 -00.12563698751 13.2354 12.5869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53002_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 53002_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 53005_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 53005_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:18:18.75 -01:13:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.035 3830639519796391680 154.57840493548 -01.22693442630 13.8072 13.3324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53055_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 53055_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:27:39.32 -00:56:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.479 3782861096709262080 156.91371739867 -00.94407356948 13.8650 13.3764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53077_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 53077_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:22:56.61 -04:47:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.138 3779408462694976896 155.73609987705 -04.78603682578 14.1357 13.6604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53081_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
Preparing report for the candidate 53081_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
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Considering the candidate 53108_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 53108_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 09:49:08.80 -06:17:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.972 3820143135121025792 147.28749638175 -06.29937227779 13.6321 13.0316 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53127_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 53127_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:30:31.79 -02:43:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.137 3781310068055068672 157.63255311862 -02.73088464459 14.1257 13.5165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53174_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 53174_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:25:43.87 +01:28:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53189_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 53189_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
**** FOUND 10:41:13.21 -00:17:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.720 3806089963473642368 160.30522743330 -00.29284269357 13.6409 12.9377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53238_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
Preparing report for the candidate 53238_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
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Considering the candidate 53274_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073
The candidate 53274_Sex-02-Q2b1x1_2026-02-26_23-29-47_20.00sec_-14.90C_LIGHT_0073 did not pass the final checks
