How to Install and Uninstall cpl-plugin-uves Package on Ubuntu 21.10 (Impish Indri)

Last updated: September 20,2024

1. Install "cpl-plugin-uves" package

Please follow the guidelines below to install cpl-plugin-uves on Ubuntu 21.10 (Impish Indri)

$ sudo apt update $ sudo apt install cpl-plugin-uves

2. Uninstall "cpl-plugin-uves" package

This guide covers the steps necessary to uninstall cpl-plugin-uves on Ubuntu 21.10 (Impish Indri):

$ sudo apt remove cpl-plugin-uves $ sudo apt autoclean && sudo apt autoremove

3. Information about the cpl-plugin-uves package on Ubuntu 21.10 (Impish Indri)

Package: cpl-plugin-uves
Architecture: amd64
Version: 6.1.3+dfsg-5
Multi-Arch: same
Priority: optional
Section: universe/science
Origin: Ubuntu
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astronomy Maintainers
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Installed-Size: 3411
Depends: libc6 (>= 2.33), libcext0 (>= 5.3.1), libcfitsio9 (>= 3.480~), libcplcore26 (>= 6.4), libcpldfs26 (>= 6.0), libcpldrs26 (>= 6.4), libcplui26 (>= 6.4), libgomp1 (>= 4.2.1), libgsl25 (>= 2.6), libqfits0
Recommends: esorex | python3-cpl
Suggests: cpl-plugin-uves-calib, cpl-plugin-uves-doc
Filename: pool/universe/c/cpl-plugin-uves/cpl-plugin-uves_6.1.3+dfsg-5_amd64.deb
Size: 962284
MD5sum: 604a18c238869200b4bd3377219108fd
SHA1: c325506f3681d71b6cf819749943399556110b92
SHA256: 86e796f9a7376867f742690afc868909218dcaa442b43473a9ef587b1fa84cd4
SHA512: 4d325d5980c52ea826408c8c65d1ce4c194e13256936ca75b7d87d0b4a86149de88147c5d0fdbd31be12d7bcda842bfb96c0cfa4d7119dc0c0f038fcc85dc948
Homepage: https://www.eso.org/sci/software/pipelines/uves
Description-en: 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.
Description-md5: 16a9c6a4730992bf3ca405af964f9be9