This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.8865,10.88,0.05,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 20260326.3865 10.88CV 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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:46:40.23 -28:47:28.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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
CO Oph,2461125.8865,11.33,0.05,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
CO Oph 20260326.3865 11.33CV 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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:55:04.26 -25:52:46.2 ;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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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,2461125.8865,12.59,0.05,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 20260326.3865 12.59CV 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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:55:21.46 -22:55:38.8 ;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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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,2461125.8865,13.12,0.05,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 20260326.3865 13.12CV 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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:57:07.53 -22:55:37.8 ;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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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,2461125.8865,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.3865 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:14:39.45 -27:40:53.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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,2461125.8865,13.73,0.05,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 20260326.3865 13.73CV 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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:12:09.02 -27:40:08.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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,2461125.8865,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.3865 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:16:22.30 -25:29:53.3 ;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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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
Gaia DR3 4114970615452724736,2461125.8865,13.88,0.05,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 4114970615452724736 20260326.3865 13.88CV 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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:17:06.96 -21:52:45.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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
V2097 Oph,2461125.8865,12.12,0.05,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
V2097 Oph 20260326.3865 12.12CV 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/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:00:01.77 -23:25:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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
ASASSN-V J170149.08-242903.0,2461125.8865,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J170149.08-242903.0 20260326.3865 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:01:49.09 -24:29:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3865 2461125.8865 11.97 16:53:25.34 -22:10:38.6
358.91780 13.51826 galactic Oph Second-epoch detections are separated by 0.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J253.3475-22.1702 | 16:53:25.34 -22:10:38.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9: CN2 1985PASP...97..465H NGC 6235
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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
ATO J253.3475-22.1702,2461125.8865,11.97,0.05,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
ATO J253.3475-22.1702 20260326.3865 11.97CV 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_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:53:25.34 -22:10:38.6 ;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_06-14-28_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_06-14-28_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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
DP Oph,2461125.8865,12.75,0.05,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
DP Oph 20260326.3865 12.75CV 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/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:57:31.31 -26:48:35.8 ;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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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
CX Oph,2461125.8865,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CX Oph 20260326.3865 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:55:48.71 -23:36:08.6 ;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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_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_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_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: 2461125.88674527 26.03.2026 09:16:44.791 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
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): 8081
Objects passed selection criteria: 8080
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 7739.25
Average stars matched: 7546 (97.503 %)
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 Thu Mar 26 04:18:54 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: 2461125.88674527 26.03.2026 09:16:44.791 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 170
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: 42 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): 112914
Objects passed selection criteria: 112739
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 101930
Average stars matched: 97979 (96.1238 %)
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 Thu Mar 26 04:20:44 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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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: 2461125.88619693
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_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits exists and is non-empty
Saving wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits to local_wcs_cache/
'wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits' -> 'local_wcs_cache/wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits'
wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits exists and is non-empty
Saving wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits to local_wcs_cache/
'wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits' -> 'local_wcs_cache/wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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 17:16:47.378 -25:59:25.11
Angular distance between the image centers 0.01 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 17:16:47.767 -25:59:51.28
Angular distance between the image centers 0.01 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 17:16:47.378 -25:59:25.11
Second-epoch second image center 17:16:47.767 -25:59:51.28
Angular distance between the image centers 0.00741 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.9d15IsPQNj
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.74kzwzHZJc
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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits &> /tmp/tmp.ZvEqF0Z4q4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits &> /tmp/tmp.HU2v3pQU4j
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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 8 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
2.6 pix fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
2.6 pix fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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
14.1 mag. fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
14.1 mag. fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.3 (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.9d15IsPQNj (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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/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.74kzwzHZJc (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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/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.ZvEqF0Z4q4 (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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.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_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=524, passed=8981
Got 8981 stars (including 8449 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat
util/solve_plate_with_UCAC5 got 8981 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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits -region wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.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.HU2v3pQU4j (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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=536, passed=8988
Got 8988 stars (including 8447 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat
util/solve_plate_with_UCAC5 got 8988 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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 924 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_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits -region wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/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_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits'
Saving fully-calibrated image wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits'
Preparing the HTML report for the field Oph-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20607.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20599_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 20599_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 20607_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 20607_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20614_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 20614_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:04:27.02 -27:04:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.239 4111795668204181760 256.11255360058 -27.06781078889 11.2847 11.0086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20619_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 20619_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:01:21.32 -28:45:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 0.316 6030068868800608512 255.33874917939 -28.75946428764 11.0071 10.1643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20621_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 20621_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:00:50.60 -27:52:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 0.420 6033276629601927040 255.21070931469 -27.88190481028 10.7209 9.6583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20623_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 20623_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:03:37.26 -27:08:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.321 4111788491365351424 255.90525369755 -27.14361689721 11.2563 10.8422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20625_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 20625_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:01:54.87 -28:11:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 5.355 6030253999070905984 255.48025872255 -28.18507102043 11.4826 10.5329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06085_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 06085_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:11:49.82 -26:39:11.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 7s
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 ####
16:46:40.23 -28:47:28.7
16:55:04.26 -25:52:46.2
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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits exists and is non-empty
wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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 17:16:47.378 -25:59:25.11
Angular distance between the image centers 0.01 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 17:16:47.767 -25:59:51.28
Angular distance between the image centers 0.01 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 17:16:47.378 -25:59:25.11
Second-epoch second image center 17:16:47.767 -25:59:51.28
Angular distance between the image centers 0.00741 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.PYN18BcgjB
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.psK8E7pJS0
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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits &> /tmp/tmp.WSHq0gNhyn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits &> /tmp/tmp.1Cqtxxv3fc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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 118 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
2.5 pix fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
2.4 pix fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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
14.1 mag. fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
14.2 mag. fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.6 (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.PYN18BcgjB (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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/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.psK8E7pJS0 (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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/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.WSHq0gNhyn (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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.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_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=6641, passed=90756
Got 90756 stars (including 84007 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat
util/solve_plate_with_UCAC5 got 90756 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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
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 934 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: 0.57"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits -region wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.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.1Cqtxxv3fc (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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=6729, passed=92556
Got 92556 stars (including 85700 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat
util/solve_plate_with_UCAC5 got 92556 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 936 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: 0.58"
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 936 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: 0.58"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits -region wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/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_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits
Saving fully-calibrated image wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.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_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits
Preparing the HTML report for the field Oph-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out121849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out157666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168097.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168136.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168160.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168173.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out124624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68045.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 22s
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: 6s
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Considering the candidate 167463_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167463_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:12:17.04 -22:03:07.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)
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Considering the candidate 167464_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167464_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:14:27.75 -25:14:56.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)
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Considering the candidate 167467_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167467_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:27:01.77 -23:09:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.315 4111466845509441664 261.75700718307 -23.15450051776 13.9148 13.0418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167480_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167480_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:32:27.50 -23:36:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 2.142 4110639570470611456 263.11420991248 -23.61556994947 13.9417 13.1713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167481_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167481_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:40:01.89 -21:54:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.672 4117244641674840192 265.00804020942 -21.90541215050 13.4372 12.3464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167484_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167484_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:17:02.82 -22:08:36.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
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Considering the candidate 167490_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167490_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:31:57.92 -27:35:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.317 4061253042819392768 262.99094409055 -27.58989989254 13.6416 12.7881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167500_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167500_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 167510_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167510_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:52:35.08 -22:02:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.892 4126235416976549632 253.14570123414 -22.04278296482 13.2905 12.4412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167511_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167511_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:14:43.37 -28:29:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.697 4107709711192330880 258.68138689882 -28.49814774276 13.6305 12.9882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167525_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167525_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:39:50.48 -22:27:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.159 4117152660657679744 264.96042299635 -22.45178848962 13.6832 13.1592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167526_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167526_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:56:21.20 -29:37:09.8 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 167528_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167528_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:42:04.53 -22:43:27.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 167532_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167532_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:36:46.98 -22:23:35.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 167533_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167533_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:39:22.40 -26:06:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.843 4061898078192787200 264.84280870147 -26.11174434140 12.5460 11.2362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167535_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167535_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:40:08.87 -22:11:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.112 4117165927916166144 265.03709116810 -22.19478740928 13.4534 12.1597 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167536_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167536_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:51:05.11 -25:52:03.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 167537_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167537_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:28:33.76 -22:28:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.898 4117703447254666240 262.14034423909 -22.48071268087 13.2337 12.4940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167538_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167538_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:05:21.78 -23:53:59.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 167545_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167545_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:54:44.99 -29:10:38.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 167546_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167546_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:47:20.98 -24:49:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 5.232 6046779766233101952 251.83861841314 -24.83043284783 13.4846 12.6299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167549_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167549_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:56:17.84 -26:31:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.125 6033652147183578368 254.07368080100 -26.52683750914 13.3416 12.6888 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167550_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167550_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:01:00.42 -29:55:49.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)
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Considering the candidate 167557_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167557_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:54:23.63 -26:49:36.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)
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Considering the candidate 167559_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167559_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:34:30.31 -28:58:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.698 4060296983096632832 263.62596407268 -28.97551345619 13.1907 12.5734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167563_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167563_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:56:06.06 -21:45:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167565_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167565_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:38:56.04 -27:50:05.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 167569_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167569_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:06:23.74 -28:29:02.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 167572_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167572_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:40:10.42 -22:29:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.697 4117139883226754432 265.04311131320 -22.48732212534 13.0157 12.3970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167574_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167574_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:18:22.63 -28:54:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 5.027 4107440124684517376 259.59576019137 -28.90412862420 12.5848 11.4531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167581_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167581_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:35:02.46 -29:20:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 4.359 4060087835370540160 263.75949187524 -29.34259662378 12.9256 12.4599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167582_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167582_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:30:30.33 -23:31:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.382 4111401184043842944 262.62537728685 -23.53246373765 13.1178 12.3580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167588_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167588_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:57:50.44 -22:12:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.864 4125996994743242112 254.46048356249 -22.20723218862 12.3324 11.7360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167589_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167589_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:42:20.86 -27:36:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.621 4060686278935094784 265.58739572012 -27.61646126040 11.9948 11.1154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167610_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167610_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:46:40.26 -28:47:28.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167627_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167627_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:39:53.40 -23:03:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 0.752 4116554736930442752 264.97229260545 -23.06658471566 11.4413 10.7485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167667_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167667_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:41:28.20 -21:56:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 2.527 4117197465747195648 265.36682882269 -21.94596320245 12.3266 11.6927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167676_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167676_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:29:08.95 -28:58:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167699_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 167699_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 167731_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167731_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:01:14.29 -25:42:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.660 4112177817210498176 255.30976525415 -25.71058138627 13.8255 11.9908 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167740_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167740_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:58:11.37 -23:31:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 0.567 4113468373308384768 254.54720327404 -23.51889499023 13.5151 11.7638 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167742_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167742_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:08:46.44 -27:53:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167751_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167751_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:54:36.27 -29:05:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.041 6032730447205208192 253.65079801953 -29.08729422868 13.2183 11.3946 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167777_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167777_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:10:26.70 -29:10:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.915 6029119444926565248 257.61098431242 -29.18179801806 12.8731 11.5342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167778_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167778_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:00:30.41 -26:45:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.710 6033413656263649920 255.12658616531 -26.75300227682 12.6994 11.4039 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167797_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167797_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:00:29.20 -26:11:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.353 4112092914302483200 255.12119846515 -26.18983116567 13.0075 11.6107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167800_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167800_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:23:15.41 -27:57:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.696 4107892646834879360 260.81304676166 -27.95814417927 13.1136 12.1768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167802_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 167802_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 167807_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167807_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:37:21.69 -25:07:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.930 4062216734716407168 264.34056196704 -25.12663831264 12.8991 10.8526 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167816_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167816_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:40:14.18 -23:16:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.823 4116536727981292672 265.05897207795 -23.27129542715 12.7093 11.1456 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167821_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167821_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:07:18.29 -28:11:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.581 6030020284138898816 256.82631947873 -28.19714964451 12.6380 11.1819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167824_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167824_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:20:14.61 -28:55:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 1.545 4059418683854676992 260.06039825884 -28.93043434497 13.7265 12.0867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167836_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167836_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:13:10.14 -30:03:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.629 6028827043544341760 258.29210652809 -30.05757387278 12.1926 10.1005 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167846_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167846_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:36:41.21 -23:37:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.619 4116418599202649472 264.17187982506 -23.62612695399 13.1217 11.7143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167854_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167854_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:29:49.83 -28:24:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167867_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167867_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:14:08.15 -28:14:33.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
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Considering the candidate 167880_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167880_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:23:44.60 -24:49:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 0.607 4110830193913300224 260.93587518438 -24.82002539968 13.1709 11.6809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167886_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167886_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:39:25.35 -22:03:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 3.407 4117218223450949760 264.85596913891 -22.06494667256 13.5875 12.4532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167896_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 167896_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 167899_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167899_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:34:58.52 -23:44:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 0.785 4116575863725248896 263.74401876003 -23.74085889007 14.1074 12.4685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167906_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167906_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:00:49.16 -27:48:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.571 6033280370476244992 255.20445086106 -27.81197024147 12.7461 11.4501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167919_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167919_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:38:20.53 -22:50:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.436 4116753022533762304 264.58585057701 -22.84430841430 13.2893 12.1432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167920_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167920_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:39:11.08 -21:50:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.869 4117235162805644800 264.79530984002 -21.84135781228 14.0761 12.3971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167941_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167941_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:40:50.47 -24:09:57.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 167969_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167969_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:25:41.00 -29:44:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.779 4059450569689770496 261.42067045684 -29.74821946686 13.3947 12.7805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167977_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167977_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:21:36.58 -26:21:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.462 4108383063364220160 260.40231120087 -26.36457731724 13.6025 11.9137 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167979_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167979_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:00:11.68 -28:20:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.174 6030163529883713920 255.04900734623 -28.34085064957 13.5305 12.6951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167994_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 167994_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:41:38.63 -22:55:26.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)
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Considering the candidate 168002_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 168002_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 168017_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168017_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:43:06.13 -21:58:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.117 4117275535457104256 265.77574441145 -21.98083639779 13.5706 12.4575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168024_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168024_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:42:33.37 -22:18:19.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 168036_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168036_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:37:54.45 -21:40:19.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)
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Considering the candidate 168037_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168037_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:24:16.47 -24:00:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.642 4111313296188241536 261.06812671060 -24.01652029579 14.0840 13.3845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168040_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168040_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:40:37.81 -21:43:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 1.983 4117253643926942848 265.15757552660 -21.73152223186 13.3340 12.2189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168043_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 168043_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 168044_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168044_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:42:16.59 -23:44:34.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 168048_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168048_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:37:55.79 -22:10:09.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)
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Considering the candidate 168051_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168051_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:33:04.11 -23:52:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.811 4110582808192792192 263.26713304520 -23.88147527993 13.9279 12.8485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168052_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168052_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:25:48.21 -29:25:36.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)
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Considering the candidate 168065_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168065_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:42:01.80 -21:40:46.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
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Considering the candidate 168076_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168076_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:25:53.10 -23:06:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 3.314 4111652083189787776 261.47045329775 -23.11658519214 13.7256 12.6683 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 168083_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168083_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:38:57.10 -22:12:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.843 4117206949039559296 264.73739717603 -22.20298110857 13.3107 12.2165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168086_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168086_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:24:33.15 -25:47:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.838 4109882934685220352 261.13795418237 -25.78586906436 13.6562 12.5949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168093_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168093_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:21:32.22 -22:38:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.533 4114657804406385152 260.38383023237 -22.63690631735 12.9450 11.7342 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168097_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168097_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:20:46.52 -25:15:43.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)
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Considering the candidate 168103_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 168103_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 168112_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168112_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:22:45.35 -24:51:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 2.013 4110827140287388032 260.68891661291 -24.86389129359 14.0720 13.3648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168124_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168124_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:08:14.01 -24:49:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.778 4112668650417021184 257.05843698670 -24.82118516632 14.0531 13.3772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168127_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168127_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:40:21.58 -22:36:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 2.721 4117134931032362752 265.08917962933 -22.60532929331 13.7044 12.5988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168128_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168128_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:22:27.97 -23:40:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.633 4111527219939054848 260.61605170988 -23.67771136388 14.1670 13.2203 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168129_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168129_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:18:11.13 -23:58:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 1.631 4111175646721007872 259.54632377631 -23.97478407405 14.0851 12.4062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168136_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168136_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:36:40.11 -21:47:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.588 4117997807140528000 264.16684008560 -21.79079725223 13.4340 12.3690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168159_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168159_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:11:46.43 -25:22:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.568 4112394116114823936 257.94324948558 -25.36939253738 13.5790 12.4984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168160_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168160_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:38:02.08 -22:59:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.504 4116726118857299200 264.50835328403 -22.99819126058 13.9229 13.2411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168168_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168168_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:25:56.21 -25:51:19.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)
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Considering the candidate 168173_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168173_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:34:29.22 -22:33:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.672 4117561271056505472 263.62199768224 -22.55151543698 13.2273 11.9616 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168200_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 168200_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:24:04.61 -25:11:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 0.362 4110052774872316544 261.01931888647 -25.19412069054 13.7134 12.6718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 157666_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 157666_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:53:19.24 -24:58:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.980 6034800483965815936 253.32986837480 -24.97143967932 13.2782 11.4257 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158474_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 158474_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:10:49.27 -30:04:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121849_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 121849_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:32:01.75 -23:23:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 0.981 4110659322938087168 263.00721346391 -23.39129059933 13.4477 11.8199 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 45520_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 45520_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:09:00.01 -28:24:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60742_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 60742_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:49:17.35 -27:12:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24051_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 24051_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:57:47.02 -29:29:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124624_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 124624_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 71997_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 71997_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:11:49.83 -26:39:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138228_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 138228_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:11:31.26 -24:28:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139759_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 139759_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 154393_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 154393_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 92031_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 92031_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:07:10.89 -25:14:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40882_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 40882_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:03:38.37 -28:37:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68045_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 68045_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 43863_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 43863_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 16:57:57.54 -28:23:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26023_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 26023_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:06:02.45 -29:28:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33974_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 33974_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:02:08.72 -28:59:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.923 6030050044033172736 255.53583813786 -28.98703468770 12.2559 10.9087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 127742_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
Preparing report for the candidate 127742_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
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Considering the candidate 73856_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 73856_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
**** FOUND 17:18:19.08 -26:34:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41836_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 41836_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 39673_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629
The candidate 39673_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629 did not pass the final checks