How to Install and Uninstall cpl-plugin-muse-calib Package on Ubuntu 20.10 (Groovy Gorilla)

Last updated: December 23,2024

1. Install "cpl-plugin-muse-calib" package

Please follow the guidelines below to install cpl-plugin-muse-calib on Ubuntu 20.10 (Groovy Gorilla)

$ sudo apt update $ sudo apt install cpl-plugin-muse-calib

2. Uninstall "cpl-plugin-muse-calib" package

This guide covers the steps necessary to uninstall cpl-plugin-muse-calib on Ubuntu 20.10 (Groovy Gorilla):

$ sudo apt remove cpl-plugin-muse-calib $ sudo apt autoclean && sudo apt autoremove

3. Information about the cpl-plugin-muse-calib package on Ubuntu 20.10 (Groovy Gorilla)

Package: cpl-plugin-muse-calib
Architecture: all
Version: 2.8.3+dfsg-1
Multi-Arch: foreign
Priority: optional
Section: universe/science
Source: cpl-plugin-muse
Origin: Ubuntu
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astro Team
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Installed-Size: 120840
Depends: cpl-plugin-muse, wget
Filename: pool/universe/c/cpl-plugin-muse/cpl-plugin-muse-calib_2.8.3+dfsg-1_all.deb
Size: 3276
MD5sum: bb5db241863dcd7d58466451aa460b2c
SHA1: 4ffef39584e8807be4af5f33d6571d123a14dbc2
SHA256: 2b0005ffc5b0c16e1b26b0431e9b32e001b26ce6779d5386d6d9c2e3396b0e66
SHA512: ea7cdd5d612bbee1ea07e2ed06cb98d4b98ab913eb6a6f29dc495fdfa9a91c77307321746ff638321595043f5d5572a89b5ec8316d289869e80e07a8acfb0e02
Homepage: https://www.eso.org/sci/software/pipelines/muse
Description-en: 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).
Description-md5: 9c007d000eb35d7a1da64bb454080c28