Source: eso-pipelines Section: science Priority: optional Maintainer: Debian Astronomy Team Uploaders: Ole Streicher Build-Depends: debhelper-compat (= 12) Standards-Version: 4.4.1 Homepage: https://www.eso.org/sci/software/pipelines/ Vcs-Git: https://salsa.debian.org/debian-astro-team/eso-pipelines.git Vcs-Browser: https://salsa.debian.org/debian-astro-team/eso-pipelines Package: eso-pipelines Architecture: all Depends: ${misc:Depends} Recommends: cpl-plugin-amber, cpl-plugin-fors, cpl-plugin-giraf, cpl-plugin-hawki, cpl-plugin-kmos, cpl-plugin-muse, cpl-plugin-naco, cpl-plugin-uves, cpl-plugin-vimos, cpl-plugin-visir, cpl-plugin-xshoo, python3-cpl | esorex Description: ESO VLT Instrument pipeline collection In collaboration with the various instrument consortia, the Pipeline Systems Department has undertaken to implement data reduction pipelines for the most commonly used VLT/VLTI instrument modes. These data reduction pipelines have three main purposes: . * Data quality control: Pipelines are used to produce the quantitative information necessary to monitor instrument performance. . * Master calibration product creation: pipelines are used to produce master calibration products (e.g. combined bias frames, super-flats, wavelength dispersion solutions). . * Science product creation: using pipeline-generated master calibration products, science products are produced for supported instrument modes (e.g. combined ISAAC jitter stacks; bias-corrected, flat-fielded FORS images, wavelength-calibrated UVES spectra). The accuracy of the science products can be limited both by the quality of the available master calibration products and by the algorithmic implementation of the pipelines themselves. In particular, adopted reduction strategies may not be suitable for all scientific goals. . This metapackage will install all ESO VLT pipelines along with the environments needed to run them (esorex, python-cpl).