This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031423059144092800,2461128.8786,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6031423059144092800 20260329.3786 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:47:38.11 -28:58:24.2 ;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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.8786,12.60,0.05,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 20260329.3786 12.60CV 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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:56:09.89 -22:57:38.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.8786,13.09,0.05,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 20260329.3786 13.09CV 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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:57:32.67 -23:04:05.5 ;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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.8786,13.43,0.05,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 20260329.3786 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:16:01.33 -27:47:28.5 ;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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.8786,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.3786 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:13:31.57 -27:51:53.8 ;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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.8786,13.54,0.05,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 20260329.3786 13.54CV 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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:17:58.74 -21:56:20.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20_00sec_-15_00C_LIGHT_0330_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20_00sec_-15_00C_LIGHT_0329_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: 2461099.00968565 27.02.2026 12:13:46.840 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
First image: 2461099.00968565 27.02.2026 12:13:46.840 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Last image: 2461128.87890039 29.03.2026 09:05:26.994 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.37
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7683
Objects passed selection criteria: 7666
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: 6628
Average stars matched: 6473.25 (97.6652 %)
Memory usage VmPeak: 114636 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 04:07:28 CDT 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: 2461099.00968565 27.02.2026 12:13:46.840 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
First image: 2461099.00968565 27.02.2026 12:13:46.840 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Last image: 2461128.87890039 29.03.2026 09:05:26.994 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 84
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.03
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: 28 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): 110184
Objects passed selection criteria: 110006
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 92671
Average stars matched: 88949 (95.9836 %)
Memory usage VmPeak: 1949896 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 04:09:31 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
SExtractor catalog cache: saved Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat to cache
SExtractor catalog cache: saved Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.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: 2461128.87828478
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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
Saving wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits to local_wcs_cache/
'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits' -> 'local_wcs_cache/wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits'
wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits exists and is non-empty
Saving wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits to local_wcs_cache/
'wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits' -> 'local_wcs_cache/wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits'
wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits exists and is non-empty
Saving wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits to local_wcs_cache/
'wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits' -> 'local_wcs_cache/wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits'
wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits exists and is non-empty
Saving wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits to local_wcs_cache/
'wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits' -> 'local_wcs_cache/wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.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 17:16:48.675 -26:00:08.00
Second-epoch image center 17:16:44.684 -26:00:44.02
Angular distance between the image centers 0.02 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 17:16:48.675 -26:00:08.00
Second-epoch image center 17:16:41.913 -26:01:27.50
Angular distance between the image centers 0.03 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 17:16:44.684 -26:00:44.02
Second-epoch second image center 17:16:41.913 -26:01:27.50
Angular distance between the image centers 0.01592 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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.PZCurA47UZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits &> /tmp/tmp.9se6tLwPza
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits &> /tmp/tmp.XejShg8fQh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits &> /tmp/tmp.hQAowc9kdb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
Found non-empty wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
The reference image (wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits) and catalog (wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat) found
'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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 7452 out of 10772 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.815328
a=0.000000 b=1.000000 c=22.815328
From vast_summary.log: estimated ref. image limiting mag.: -8.37
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
2.1 pix Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
2.5 pix fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
2.5 pix fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
Limiting magnitude estimates:
14.4 mag. Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
14.4 mag. Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
13.8 mag. fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
13.8 mag. fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.0 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.PZCurA47UZ (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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits' -> 'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=949, passed=10772
Got 10772 stars (including 9801 good ones) from the SExtractor catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 10772 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 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: 0.36"
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 928 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: 0.36"
Excluding outliers - 922 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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.9se6tLwPza (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/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits' -> 'wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS-calibrated image found: wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Checking if the catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS catalog name: wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=936, passed=10621
Got 10621 stars (including 9668 good ones) from the SExtractor catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat
util/solve_plate_with_UCAC5 got 10621 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 925 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 - 919 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits -region wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.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.XejShg8fQh (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=427, passed=6190
Got 6190 stars (including 5755 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat
util/solve_plate_with_UCAC5 got 6190 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 923 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits -region wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.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.hQAowc9kdb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=426, passed=6250
Got 6250 stars (including 5820 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat
util/solve_plate_with_UCAC5 got 6250 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 922 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits -region wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits'
Saving fully-calibrated image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits'
Saving fully-calibrated image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits'
Saving fully-calibrated image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits'
Preparing the HTML report for the field Oph-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20592.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 20592_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
Preparing report for the candidate 20592_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06085_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 06085_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:11:49.80 -26:39:11.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Oph-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:47:38.11 -28:58:24.2
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
SExtractor catalog cache: saved Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat to cache
SExtractor catalog cache: saved Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Creating symlink local_wcs_cache/wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits exists and is non-empty
wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits exists and is non-empty
wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.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 17:16:48.675 -26:00:08.00
Second-epoch image center 17:16:44.684 -26:00:44.02
Angular distance between the image centers 0.02 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 17:16:48.675 -26:00:08.00
Second-epoch image center 17:16:41.913 -26:01:27.50
Angular distance between the image centers 0.03 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 17:16:44.684 -26:00:44.02
Second-epoch second image center 17:16:41.913 -26:01:27.50
Angular distance between the image centers 0.01592 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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.dT6HBZ9KRs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits &> /tmp/tmp.zt3EM003w6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits &> /tmp/tmp.JcsmVJNvzW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits &> /tmp/tmp.mvwyBsv8wj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
Found non-empty wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
The reference image (wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits) and catalog (wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat) found
'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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 9812 out of 143168 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.596166
a=0.000000 b=1.000000 c=22.596166
From vast_summary.log: estimated ref. image limiting mag.: -8.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.57
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 65 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
1.8 pix Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
2.3 pix fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
2.3 pix fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
Limiting magnitude estimates:
14.6 mag. Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
14.5 mag. Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
13.8 mag. fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
13.9 mag. fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.dT6HBZ9KRs (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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits' -> 'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=11615, passed=143155
Got 143155 stars (including 131260 good ones) from the SExtractor catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 143155 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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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.zt3EM003w6 (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/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits' -> 'wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS-calibrated image found: wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Checking if the catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS catalog name: wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=11364, passed=142792
Got 142792 stars (including 131150 good ones) from the SExtractor catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat
util/solve_plate_with_UCAC5 got 142792 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 941 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 - 937 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits -region wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.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.JcsmVJNvzW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=3852, passed=69788
Got 69788 stars (including 65846 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat
util/solve_plate_with_UCAC5 got 69788 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 933 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: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 930 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_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits -region wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.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.mvwyBsv8wj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=3796, passed=69606
Got 69606 stars (including 65711 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat
util/solve_plate_with_UCAC5 got 69606 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
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: 0.55"
Estimated accuracy of the plate solution: 0.60"
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_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits -region wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Saving fully-calibrated image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Saving fully-calibrated image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-04-33_20.00sec_-15.00C_LIGHT_0329.fits
Saving fully-calibrated image wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-08-Q2b1x1_040602_TTUQ2b1x1_8683_YTnh6elF/wcs_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330.fits
Preparing the HTML report for the field Oph-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out167475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out167486.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out167687.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out167674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167852.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 3s
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Considering the candidate 167475_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167475_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:04:42.79 -26:42:32.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)
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Considering the candidate 167486_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167486_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:42:24.24 -21:56:57.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)
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Considering the candidate 167490_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167490_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:15:09.65 -26:55:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.503 4108986489076003968 258.79023101994 -26.92508292615 10.7640 9.3830 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167491_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167491_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:56:06.06 -21:45:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167495_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167495_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:40:10.28 -22:29:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167500_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167500_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:03:36.18 -26:57:19.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 167501_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167501_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:02:21.80 -29:53:57.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)
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Considering the candidate 167502_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167502_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:38:29.71 -22:53:08.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)
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Considering the candidate 167505_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167505_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:15:41.78 -23:39:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.379 4114154773479940864 258.92446137106 -23.65633632630 12.6728 11.6538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167512_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167512_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:02:58.66 -28:57:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.941 6029886762189679488 255.74556934388 -28.95440745677 12.9921 11.2476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167519_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167519_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:47:15.99 -23:43:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 4.215 6047183458786753536 251.81599718741 -23.72121444253 12.1794 10.8600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167533_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167533_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:57:50.53 -22:12:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167534_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167534_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:13:23.20 -23:11:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167536_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167536_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:05:50.32 -29:44:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 3.136 6029037325152979712 256.46002442568 -29.73474158030 9.8898 8.3664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167554_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167554_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:47:38.15 -28:58:24.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167646_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167646_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:29:09.01 -28:58:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167674_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
Preparing report for the candidate 167674_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
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Considering the candidate 167680_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167680_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:58:11.35 -23:31:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167685_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167685_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:58:58.89 -28:33:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.108 6030133602553872512 254.74425760382 -28.56163773007 12.7863 12.2354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167687_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167687_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:54:58.26 -29:50:19.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 167688_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167688_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:04:02.01 -25:40:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167693_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167693_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:55:10.88 -21:56:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167699_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167699_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:58:28.65 -29:23:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.882 6029673388213104128 254.61917679515 -29.39215948855 12.2216 11.1072 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167700_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167700_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:54:59.44 -29:50:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.314 6029585947043907968 253.74835824330 -29.83799623850 12.9313 12.0217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167702_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167702_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:08:46.47 -27:53:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167714_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167714_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:54:36.27 -29:05:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167716_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167716_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:08:23.26 -29:20:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.738 6029137067056578304 257.09774435697 -29.34423144208 13.1212 12.1668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167735_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167735_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:00:29.32 -26:11:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167746_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167746_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:00:30.42 -26:45:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167749_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167749_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:01:14.31 -25:42:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167752_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167752_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:07:18.30 -28:11:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167757_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167757_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:10:26.74 -29:10:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167770_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167770_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:02:46.34 -26:14:44.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 167774_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167774_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:37:21.68 -25:07:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167776_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
Preparing report for the candidate 167776_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
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Considering the candidate 167802_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167802_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:23:44.58 -24:49:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167810_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167810_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:23:11.62 -25:23:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 3.502 4109955841654642816 260.79800720341 -25.38995518591 13.6138 13.0489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167811_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167811_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:40:14.15 -23:16:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167816_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167816_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:29:49.83 -28:24:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167819_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
Preparing report for the candidate 167819_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
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Considering the candidate 167820_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167820_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:20:14.59 -28:55:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167839_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167839_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:18:11.16 -23:58:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167843_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
Preparing report for the candidate 167843_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
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Considering the candidate 167850_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167850_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:21:32.13 -22:38:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167852_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
Preparing report for the candidate 167852_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
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Considering the candidate 167874_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 167874_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:21:36.66 -26:21:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154393_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 154393_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:53:25.30 -22:10:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121849_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 121849_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:32:01.75 -23:23:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45520_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 45520_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:08:59.96 -28:24:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47833_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 47833_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:06:49.99 -28:15:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60742_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 60742_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:49:17.36 -27:12:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24051_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 24051_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:57:47.02 -29:29:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139759_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 139759_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:01:49.07 -24:29:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138228_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 138228_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:11:31.26 -24:28:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124624_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 124624_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:00:01.76 -23:25:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71997_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 71997_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:11:49.82 -26:39:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92031_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 92031_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:07:10.88 -25:14:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158474_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 158474_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:10:49.25 -30:04:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157666_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 157666_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:53:19.23 -24:58:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26023_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 26023_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:06:02.53 -29:28:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33974_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 33974_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:02:08.67 -28:59:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43863_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 43863_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:57:57.49 -28:23:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127742_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 127742_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 16:55:48.70 -23:36:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73856_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 73856_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks
**** FOUND 17:18:19.00 -26:34:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39673_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330
The candidate 39673_fd_Oph-08-Q2b1x1_2026-03-29_04-05-26_20.00sec_-15.00C_LIGHT_0330 did not pass the final checks