Source: cpl-plugin-visir Maintainer: Debian Astronomy Team Uploaders: Ole Streicher Section: science Priority: optional Build-Depends: debhelper-compat (= 13), libcpl-dev, python3, python3-astropy, python3-cpl, Build-Depends-Indep: dh-sequence-sphinxdoc, python3-sphinx Standards-Version: 4.5.0 Vcs-Browser: https://salsa.debian.org/debian-astro-team/cpl-plugin-visir Vcs-Git: https://salsa.debian.org/debian-astro-team/cpl-plugin-visir.git Homepage: https://www.eso.org/sci/software/pipelines/visir Rules-Requires-Root: no Package: cpl-plugin-visir Architecture: any Multi-Arch: same Depends: ${misc:Depends}, ${shlibs:Depends}, swarp Recommends: esorex | python3-cpl Suggests: cpl-plugin-visir-calib, cpl-plugin-visir-doc Description: ESO data reduction pipeline for the VISIR instrument This is the data reduction pipeline for the Visir instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . The VLT spectrometer and imager for the mid-infrared (VISIR) was built by CEA/DAPNIA/SAP and NFRA/ASTRON, and is located at the Cassegrain focus of UT3. It provides diffraction-limited imaging at high sensitivity in the two mid infrared (MIR) atmospheric windows: the N band between 8 to 13μm and the Q band between 16.5 and 24.5μm, respectively. In addition, it features a long-slitspectrometer with a range of spectral resolutions between 150 and 30000. Package: cpl-plugin-visir-doc Architecture: all Multi-Arch: foreign Section: doc Depends: ${misc:Depends} Description: ESO data reduction pipeline documentation for the VISIR instrument This package contains the HTML documentation and manpages for the data reduction pipeline for the Visir instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). Package: cpl-plugin-visir-calib Architecture: all Multi-Arch: foreign Section: contrib/science Depends: ${misc:Depends}, cpl-plugin-visir, wget Description: ESO data reduction pipeline calibration data downloader for VISIR This package downloads calibration and other static data of the data reduction pipeline for the Visir instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . The VLT spectrometer and imager for the mid-infrared (VISIR) was built by CEA/DAPNIA/SAP and NFRA/ASTRON, and is located at the Cassegrain focus of UT3. It provides diffraction-limited imaging at high sensitivity in the two mid infrared (MIR) atmospheric windows: the N band between 8 to 13μm and the Q band between 16.5 and 24.5μm, respectively. In addition, it features a long-slitspectrometer with a range of spectral resolutions between 150 and 30000.