Source: cpl-plugin-muse Section: science Priority: optional Maintainer: Debian Astro Team Uploaders: Ole Streicher Build-Depends: debhelper (>= 11), libcpl-dev (>= 6.5), python3, python3-astropy, python3-cpl, python3-sphinx Standards-Version: 4.2.1 Homepage: https://www.eso.org/sci/software/pipelines/muse Vcs-Git: https://salsa.debian.org/debian-astro-team/cpl-plugin-muse.git Vcs-Browser: https://salsa.debian.org/debian-astro-team/cpl-plugin-muse Package: cpl-plugin-muse Architecture: any Depends: ${misc:Depends}, ${shlibs:Depends} Recommends: esorex|python3-cpl|python-cpl Suggests: cpl-plugin-muse-calib, cpl-plugin-muse-doc Multi-Arch: same Description: ESO data reduction pipeline for the MUSE instrument This is the data reduction pipeline for the Muse instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . MUSE, the Multi-Unit Spectroscopic Explorer, is an Integral Field Spectrograph located at the Nasmyth B focus of Yepun, the VLT UT4 telescope. It has a modular structure composed of 24 identical IFU modules that together sample, in Wide Field Mode (WFM), a near-contiguous 1 squared arcmin field of view. Spectrally the instrument samples almost the full optical domain with a mean resolution of 3000. Spatially, the instrument samples the sky with 0.2 arcseconds spatial pixels in the currently offered Wide Field Mode with natural seeing (WFM-noAO). Package: cpl-plugin-muse-doc Architecture: all Multi-Arch: foreign Depends: ${misc:Depends} Section: doc Description: ESO data reduction pipeline documentation for MUSE This package contains the HTML documentation and manpages for the data reduction pipeline for the Muse instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). Package: cpl-plugin-muse-calib Architecture: all Multi-Arch: foreign Depends: ${misc:Depends}, cpl-plugin-muse, wget Section: contrib/science Description: ESO data reduction pipeline calibration data downloader for MUSE This package downloads calibration and other static data of the data reduction pipeline for the Muse instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . MUSE, the Multi-Unit Spectroscopic Explorer, is an Integral Field Spectrograph located at the Nasmyth B focus of Yepun, the VLT UT4 telescope. It has a modular structure composed of 24 identical IFU modules that together sample, in Wide Field Mode (WFM), a near-contiguous 1 squared arcmin field of view. Spectrally the instrument samples almost the full optical domain with a mean resolution of 3000. Spatially, the instrument samples the sky with 0.2 arcseconds spatial pixels in the currently offered Wide Field Mode with natural seeing (WFM-noAO).