This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX
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
ASAS J173835-0459.4,2461098.8839,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J173835-0459.4 20260227.3839 11.23CV 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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:38:33.92 -04:59:33.8 ;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-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3839* 17 37 46.67 -13 37 02.7 12.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173747.12-133707.2,2461098.8839,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173747.12-133707.2 20260227.3839 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:37:46.67 -13:37:02.7 ;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-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3839 2461098.8839 11.87 17:39:31.91 -14:39:02.8
11.49895 8.65087 galactic Ser Second-epoch detections are separated by 3.1" and 3.0 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 | Gaia DR3 4149248955591882112 | 17:39:32.33 -14:39:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
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!
TCP 2026 02 27.3839* 17 39 31.91 -14 39 02.8 11.9 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4149248955591882112,2461098.8839,11.87,0.05,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 4149248955591882112 20260227.3839 11.87CV 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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:39:31.91 -14:39:02.8 ;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-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.8839,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.3839 12.42CV 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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:46:40.02 -12:27:12.7 ;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-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3839 2461098.8839 12.55 17:38:33.40 -05:02:34.5
19.82796 13.71633 galactic Oph Second-epoch detections are separated by 0.6" and 3.0 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 J264.6435-05.0420 | 17:38:33.75 -05:02:28.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
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 J264.6435-05.0420,2461098.8839,12.55,0.05,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 J264.6435-05.0420 20260227.3839 12.55CV 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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:38:33.40 -05:02:34.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3839* 17 38 36.73 -12 46 59.0 12.8 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0605 Ser,2461098.8839,12.82,0.05,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
V0605 Ser 20260227.3839 12.82CV 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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:38:36.73 -12:46:59.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3839* 17 29 41.05 -14 33 59.9 13.0 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.8839,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260227.3839 12.96CV 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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:29:41.05 -14:33:59.9 ;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-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_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
NSVS J1739199-064120,2461098.8839,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1739199-064120 20260227.3839 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:39:19.51 -06:41:16.8 ;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-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.8839,13.66,0.05,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 20260227.3839 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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:43:33.92 -10:28:34.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_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
V1055 Oph,2461098.8839,10.55,0.05,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
V1055 Oph 20260227.3839 10.55CV 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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:57:52.09 -09:32:32.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.99252847 18.01.2026 11:49:04.460 /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
First image: 2461058.99252847 18.01.2026 11:49:04.460 /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
Last image: 2461098.88414882 27.02.2026 09:13:00.458 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.25
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 3978
Objects passed selection criteria: 3974
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: 3559.75
Average stars matched: 3450.25 (96.9239 %)
Memory usage VmPeak: 110648 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 7 15:05:07 CST 2026
VaST build number 1.0rc88-348-g7938252d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Mar 10 17:32:44 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: 2461058.99252847 18.01.2026 11:49:04.460 /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
First image: 2461058.99252847 18.01.2026 11:49:04.460 /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
Last image: 2461098.88414882 27.02.2026 09:13:00.458 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 157
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.93
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: 10 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): 35727
Objects passed selection criteria: 35691
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: 32629.2
Average stars matched: 30909.2 (94.7287 %)
Memory usage VmPeak: 139720 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 7 15:05:07 CST 2026
VaST build number 1.0rc88-348-g7938252d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Mar 10 17:33:39 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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
SExtractor catalog cache: saved Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat to cache
SExtractor catalog cache: saved Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461098.88363647
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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits exists and is non-empty
Saving wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits to local_wcs_cache/
'wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits' -> 'local_wcs_cache/wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits'
wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits exists and is non-empty
Saving wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits to local_wcs_cache/
'wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits' -> 'local_wcs_cache/wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits'
wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits exists and is non-empty
Saving wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits to local_wcs_cache/
'wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits' -> 'local_wcs_cache/wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits'
wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits exists and is non-empty
Saving wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits to local_wcs_cache/
'wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits' -> 'local_wcs_cache/wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits'
The image scale is 5.92"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:08:44.680 -10:03:02.32
Second-epoch image center 17:08:34.957 -10:00:16.00
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:08:44.680 -10:03:02.32
Second-epoch image center 17:08:33.963 -10:00:23.70
Angular distance between the image centers 0.06 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 17:08:34.957 -10:00:16.00
Second-epoch second image center 17:08:33.963 -10:00:23.70
Angular distance between the image centers 0.00460 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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits &> /tmp/tmp.CVNl7WgWXM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits &> /tmp/tmp.Cs2AgnbwhS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits &> /tmp/tmp.j7PHbSqLEm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits &> /tmp/tmp.ZHLPlvTMs6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits and wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits and wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat
Found non-empty wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits and wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat
The reference image (wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits) and catalog (wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat) found
'wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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 2841 out of 4144 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.595432
a=0.000000 b=1.000000 c=22.595432
From vast_summary.log: estimated ref. image limiting mag.: -8.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.35
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.35
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
2.4 pix Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
2.5 pix fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
2.5 pix fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
Limiting magnitude estimates:
14.3 mag. Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
14.4 mag. Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
13.9 mag. fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
13.9 mag. fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.CVNl7WgWXM (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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits' -> 'wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
WCS_IMAGE_NAME=wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
WCS-calibrated image found: wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
Checking if the catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat corresponding to the image wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits alredy exist and is non-empty...
Catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat corresponding to the image wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
WCS catalog name: wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=208, passed=4144
Got 4144 stars (including 3933 good ones) from the SExtractor catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat
util/solve_plate_with_UCAC5 got 4144 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.5'
Seting catalog search parameters based on the expected field of view 945.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013132 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010506 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 940 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: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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: 0.51"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits -region wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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.Cs2AgnbwhS (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-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.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-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.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-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits' -> 'wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
WCS-calibrated image found: wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
Checking if the catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
WCS catalog name: wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=229, passed=4361
Got 4361 stars (including 4126 good ones) from the SExtractor catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 4361 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits -region wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.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.j7PHbSqLEm (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
WCS-calibrated image found: wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
Checking if the catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat corresponding to the image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat corresponding to the image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
WCS catalog name: wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=162, passed=2895
Got 2895 stars (including 2731 good ones) from the SExtractor catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat
util/solve_plate_with_UCAC5 got 2895 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.75"
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: 0.75"
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 934 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits -region wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.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.ZHLPlvTMs6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
WCS_IMAGE_NAME=wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
WCS-calibrated image found: wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
Checking if the catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat corresponding to the image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat corresponding to the image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
WCS catalog name: wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=164, passed=2932
Got 2932 stars (including 2766 good ones) from the SExtractor catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat
util/solve_plate_with_UCAC5 got 2932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 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: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.74"
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 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.74"
Estimated accuracy of the plate solution: 0.74"
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_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits -region wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits'
Saving fully-calibrated image wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits'
Saving fully-calibrated image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits'
Saving fully-calibrated image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits'
Preparing the HTML report for the field Oph-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out02355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20425.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20410_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 20410_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:00:29.50 -12:15:49.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20421_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 20421_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:28:53.84 -05:59:06.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20423_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 20423_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:35:03.04 -05:58:08.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20425_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
Preparing report for the candidate 20425_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02355_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 02355_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 16:57:52.08 -09:32:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.36, MAG_FAINT_SEARCH_LIMIT=11.34)GAIADR2_OUTPUT=# 1.240 4336170085503609472 254.46669240270 -09.54203145377 10.0196 8.3815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Oph-05-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 ####
17:38:33.92 -04:59:33.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
SExtractor catalog cache: saved Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat to cache
SExtractor catalog cache: saved Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
Creating symlink local_wcs_cache/wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits exists and is non-empty
wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits exists and is non-empty
wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits exists and is non-empty
wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits exists and is non-empty
The image scale is 5.92"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:08:44.680 -10:03:02.32
Second-epoch image center 17:08:34.957 -10:00:16.00
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:08:44.680 -10:03:02.32
Second-epoch image center 17:08:33.963 -10:00:23.70
Angular distance between the image centers 0.06 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 17:08:34.957 -10:00:16.00
Second-epoch second image center 17:08:33.963 -10:00:23.70
Angular distance between the image centers 0.00460 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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits &> /tmp/tmp.TP1QLkwdnV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits &> /tmp/tmp.S3LaPsit0y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits &> /tmp/tmp.dwe9wcpMOi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits &> /tmp/tmp.aXEanjfljc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits and wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits and wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat
Found non-empty wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits and wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat
The reference image (wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits) and catalog (wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat) found
'wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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 3570 out of 38662 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.384048
a=0.000000 b=1.000000 c=22.384048
From vast_summary.log: estimated ref. image limiting mag.: -7.93
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 132 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
2.3 pix Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
2.4 pix fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
2.4 pix fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
Limiting magnitude estimates:
14.5 mag. Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
14.5 mag. Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
14.1 mag. fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
14.1 mag. fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.TP1QLkwdnV (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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits' -> 'wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
WCS_IMAGE_NAME=wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
WCS-calibrated image found: wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
Checking if the catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat corresponding to the image wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits alredy exist and is non-empty...
Catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat corresponding to the image wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
WCS catalog name: wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1724, passed=38661
Got 38661 stars (including 36880 good ones) from the SExtractor catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat
util/solve_plate_with_UCAC5 got 38661 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.5'
Seting catalog search parameters based on the expected field of view 945.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013132 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010506 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits -region wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.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.S3LaPsit0y (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-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.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-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.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-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits' -> 'wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
WCS-calibrated image found: wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
Checking if the catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
WCS catalog name: wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1837, passed=41287
Got 41287 stars (including 39375 good ones) from the SExtractor catalog wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 41287 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits -region wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.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.dwe9wcpMOi (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
WCS-calibrated image found: wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
Checking if the catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat corresponding to the image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat corresponding to the image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
WCS catalog name: wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=746, passed=25733
Got 25733 stars (including 24953 good ones) from the SExtractor catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat
util/solve_plate_with_UCAC5 got 25733 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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: 0.69"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits -region wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.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.aXEanjfljc (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
WCS_IMAGE_NAME=wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
WCS-calibrated image found: wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
Checking if the catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat corresponding to the image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat corresponding to the image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
WCS catalog name: wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=763, passed=26034
Got 26034 stars (including 25236 good ones) from the SExtractor catalog wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat
util/solve_plate_with_UCAC5 got 26034 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
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: 0.67"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits -region wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.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-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits
Saving fully-calibrated image wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/wcs_Oph-05-Q2b1x1_2026-01-18_05-54-29_20.00sec_-15.00C_LIGHT_0000.fits
Saving fully-calibrated image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits
Saving fully-calibrated image wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits
Preparing the HTML report for the field Oph-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out50014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out21404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56555.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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 56265_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56265_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 16:39:22.24 -08:36:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.679 4338952919369022464 249.84222555480 -08.61366496520 13.5609 12.7084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56267_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56267_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:03:10.31 -08:26:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.085 4336729977439073792 255.79406310792 -08.44561133281 12.0456 10.5018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56273_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56273_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:25:18.87 -11:45:18.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
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Considering the candidate 56274_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56274_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:26:05.42 -12:43:04.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)
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Considering the candidate 56277_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56277_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:19:01.87 -14:36:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.646 4138004280197341952 259.75674875210 -14.60705687441 12.1344 11.0696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56283_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
Preparing report for the candidate 56283_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
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Considering the candidate 56286_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
Preparing report for the candidate 56286_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
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Considering the candidate 56287_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56287_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 56296_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56296_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:36:00.27 -14:52:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56304_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56304_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:37:27.09 -14:37:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56306_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56306_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:38:33.97 -04:59:34.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 56307_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56307_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:32:49.43 -15:00:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56317_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56317_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 56318_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56318_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:37:10.56 -14:55:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56319_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56319_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 56325_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56325_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:34:05.59 -13:10:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56328_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56328_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 56331_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56331_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 56334_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56334_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:38:18.14 -14:06:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56343_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56343_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 56348_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56348_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 56349_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
Preparing report for the candidate 56349_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
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Considering the candidate 56350_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56350_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 16:46:31.58 -11:47:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.097 4334030745111684096 251.63098955374 -11.79273766057 12.3559 10.5239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56352_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56352_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:23:08.44 -07:06:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.516 4360295058541704192 260.78559115799 -07.11414105691 12.2159 11.4041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56353_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56353_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:21:37.63 -14:03:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56357_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56357_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:34:42.92 -11:13:30.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 56358_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56358_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:37:24.35 -14:28:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 5.388 4137306884911505152 264.35001520435 -14.47900864503 10.6786 10.1068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56359_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56359_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:23:45.88 -11:46:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.696 4141882399449687296 260.94140082152 -11.77121703147 12.7573 10.7666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56364_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
Preparing report for the candidate 56364_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
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Considering the candidate 56366_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56366_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:18:50.09 -15:00:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56368_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56368_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 56369_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56369_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 56377_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56377_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 56379_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56379_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 16:47:06.60 -08:26:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.457 4338090936613271552 251.77751508518 -08.44865181123 12.6967 12.0666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56380_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
Preparing report for the candidate 56380_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
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Considering the candidate 56382_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56382_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 56385_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56385_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 56386_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56386_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 56387_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56387_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:19:19.73 -06:38:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.704 4360547499538067712 259.83217230100 -06.64638920031 11.9815 10.0031 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56392_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56392_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:25:21.29 -08:49:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 3.781 4167618423301011072 261.33764569761 -08.83091631919 12.1522 10.9691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56393_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56393_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:14:06.29 -08:23:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.886 4359815151779477248 258.52614175748 -08.38831362748 12.7517 12.0331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56394_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
Preparing report for the candidate 56394_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
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Considering the candidate 56396_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56396_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:35:24.76 -13:36:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.164 4161618014683101952 263.85342647332 -13.61578622785 13.5781 11.4587 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56398_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56398_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 56399_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56399_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 56400_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56400_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 56403_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56403_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 56404_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56404_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:36:57.10 -10:22:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56406_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56406_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 56409_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56409_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 56412_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56412_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 56413_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56413_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 56417_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56417_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:30:53.91 -14:47:31.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)
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Considering the candidate 56429_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56429_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 56432_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
Preparing report for the candidate 56432_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
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Considering the candidate 56435_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56435_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 56436_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56436_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 56439_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56439_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 56441_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56441_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:19:50.82 -14:58:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.237 4137769878067414144 259.96205662175 -14.97736881288 12.1135 10.8484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56443_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56443_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:36:14.65 -06:19:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 5.606 4169874728536899840 264.06236491618 -06.32669398102 13.2822 11.6942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56444_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56444_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 56449_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56449_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 56450_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56450_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:25:28.29 -14:29:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.252 4137871960842138112 261.36813865253 -14.48542207523 11.1433 9.5579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56452_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56452_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 56457_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56457_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:24:30.72 -10:54:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.016 4166152808660063360 261.12809438873 -10.90289215407 11.8650 10.2312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56458_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56458_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 56463_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56463_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:39:36.78 -12:56:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.342 4161592107480128128 264.90391760777 -12.94661270451 12.0072 10.5860 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56464_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56464_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 16:37:24.35 -14:51:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.369 4326993114780099200 249.35082509573 -14.85985249514 12.7107 11.8635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56466_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56466_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 56472_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56472_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:18:07.80 -11:04:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.211 4142904391203971072 259.53245730849 -11.08309788396 13.5221 11.4978 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56473_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56473_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 56474_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56474_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 56475_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56475_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:22:05.87 -13:46:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.201 4138166870481179776 260.52424702898 -13.77206862452 12.0222 10.4928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56476_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56476_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 56477_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56477_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 56479_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56479_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 56480_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56480_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 56483_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56483_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 56488_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56488_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 56489_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56489_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 16:37:29.47 -11:51:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 0.171 4331014715997168896 249.37281021675 -11.85187290328 13.2859 12.5454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56490_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56490_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 56491_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56491_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:14:30.47 -11:43:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.998 4142769808405392256 258.62713410163 -11.71927283902 13.4142 11.1634 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56492_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56492_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 56494_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56494_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 56495_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56495_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 56497_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56497_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 56499_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56499_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:23:46.85 -15:06:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.679 4137071314528159616 260.94614869146 -15.11402473560 11.0941 9.5977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56500_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56500_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 56501_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56501_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 56505_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56505_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 56506_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56506_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 56507_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56507_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 56510_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56510_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:18:56.22 -09:32:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.394 4167293895570219264 259.73490673398 -09.54106482015 13.0461 10.8581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56513_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56513_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 56519_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56519_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:15:05.33 -09:23:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.253 4359491276883257344 258.77189620378 -09.39724554329 12.5272 11.1441 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56521_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56521_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 56530_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56530_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 56531_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56531_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 56534_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56534_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:04:59.42 -09:55:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.769 4335253951798288384 256.24713901352 -09.92763746879 12.5455 11.1661 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56535_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56535_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 56537_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56537_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 56538_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56538_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 56540_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56540_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 56541_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56541_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 56548_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56548_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 56555_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
Preparing report for the candidate 56555_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
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Considering the candidate 56560_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56560_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 56562_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56562_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:01:00.42 -09:02:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.403 4336121500832560640 255.25185499570 -09.04582029266 13.9595 12.1090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56567_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56567_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 56568_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56568_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 16:45:37.09 -13:17:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.532 4327580636245672832 251.40443545836 -13.28966124312 13.3950 12.2798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56571_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56571_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 56573_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56573_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 56576_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56576_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 56578_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56578_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:17:58.30 -11:24:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.134 4142138787514687872 259.49267030636 -11.41149229960 12.6679 11.3238 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56579_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56579_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:04:45.77 -07:44:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.011 4336882642053457536 256.19099163197 -07.74362766003 14.1514 12.5452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56583_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56583_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 56586_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56586_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:00:14.61 -09:32:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.008 4336067457260352768 255.06040815263 -09.54248149356 13.6652 12.7518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56588_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56588_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 56594_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56594_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 56599_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56599_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 56601_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56601_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 56609_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56609_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 56614_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56614_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 56616_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56616_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 56618_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56618_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:14:18.43 -07:21:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.036 4360038460014732032 258.57666154862 -07.36279817849 13.1079 11.8700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56619_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 56619_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 50014_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 50014_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:04:49.38 -07:45:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.538 4336882362879602944 256.20567029439 -07.76412679778 12.4206 11.4157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 29161_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 29161_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:28:53.81 -05:59:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29016_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 29016_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:35:02.99 -05:58:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11278_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 11278_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks
**** FOUND 17:00:29.54 -12:15:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55905_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167
The candidate 55905_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167 did not pass the final checks