Source: cpl-plugin-uves Section: science Priority: optional Maintainer: Debian Astronomy Maintainers Uploaders: Ole Streicher Build-Depends: debhelper (>= 11), libcfitsio-dev, libcpl-dev (>= 5.3.1), libqfits-dev, python3, python3-astropy, python3-cpl, python3-sphinx Standards-Version: 4.1.4 Homepage: https://www.eso.org/sci/software/pipelines/uves Vcs-Git: https://salsa.debian.org/debian-astro-team/cpl-plugin-uves.git Vcs-Browser: https://salsa.debian.org/debian-astro-team/cpl-plugin-uves Package: cpl-plugin-uves Architecture: any Depends: ${misc:Depends}, ${shlibs:Depends} Recommends: esorex | python3-cpl Suggests: cpl-plugin-uves-calib, cpl-plugin-uves-doc Multi-Arch: same Description: ESO data reduction pipeline for the UVES instrument This is the data reduction pipeline for the UVES instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . UVES is a cross-dispersed echelle spectrograph designed to operate with high efficiency from the atmospheric cut-off at 300 nm to the long wavelength limit of the CCD detectors (about 1100 nm). The light beam from the telescope is split in two arms (UV to Blue, and Visual to Red) within the instrument. The two arms can be operated separately, or in parallel via a dichroic beam splitter. The resolving power is about 40,000 when a 1-arcsec slit is used. The maximum (two-pixel) resolution is 80,000 or 110,000 in the Blue- and the Red Arm, respectively. Package: cpl-plugin-uves-doc Architecture: all Multi-Arch: foreign Depends: ${misc:Depends} Section: doc Description: ESO data reduction pipeline documentation for UVES This package contains the HTML documentation and manpages for the data reduction pipeline for the UVES instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). Package: cpl-plugin-uves-calib Architecture: all Multi-Arch: foreign Depends: ${misc:Depends}, cpl-plugin-uves, wget Section: contrib/science Description: ESO data reduction pipeline calibration data downloader for UVES This package downloads calibration and other static data of the data reduction pipeline for the UVES instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO).