Source: cpl-plugin-naco Maintainer: Debian Astronomy Maintainers Uploaders: Ole Streicher Section: science Priority: optional Build-Depends: debhelper-compat (= 13), libgsl-dev, libcpl-dev, python3, python3-astropy, python3-cpl Build-Depends-Indep: dh-sequence-sphinxdoc, python3-sphinx Standards-Version: 4.6.1 Vcs-Browser: https://salsa.debian.org/debian-astro-team/cpl-plugin-naco Vcs-Git: https://salsa.debian.org/debian-astro-team/cpl-plugin-naco.git Homepage: https://www.eso.org/sci/software/pipelines/naco Rules-Requires-Root: no Package: cpl-plugin-naco Architecture: any Multi-Arch: same Depends: ${misc:Depends}, ${shlibs:Depends} Recommends: esorex | python3-cpl Suggests: cpl-plugin-naco-calib, cpl-plugin-naco-doc Description: ESO data reduction pipeline for the NaCo instrument This is the data reduction pipeline for the NaCo instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . NaCo is short for NAOS-CONICA. It was installed at the Nasmyth B focus of UT4 from 2001 through 2013. In 2014 it was reinstalled on UT1 at the Nasmyth A. It provides adaptive optics assisted imaging, imaging polarimetry, coronography and spectroscopy, in the 1-5 micron range. Package: cpl-plugin-naco-doc Architecture: all Multi-Arch: foreign Section: doc Depends: ${misc:Depends} Description: ESO data reduction pipeline documentation for NaCo This package contains the HTML documentation and manpages for the data reduction pipeline for the NaCo instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). Package: cpl-plugin-naco-calib Architecture: all Multi-Arch: foreign Section: contrib/science Depends: ${misc:Depends}, cpl-plugin-naco, wget Description: ESO data reduction pipeline NaCo calibration data downloader This package downloads calibration and other static data of the data reduction pipeline for the NaCo instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . NaCo is short for NAOS-CONICA. It was installed at the Nasmyth B focus of UT4 from 2001 through 2013. In 2014 it was reinstalled on UT1 at the Nasmyth A. It provides adaptive optics assisted imaging, imaging polarimetry, coronography and spectroscopy, in the 1-5 micron range.