How to Install and Uninstall cpl-plugin-uves Package on Ubuntu 21.04 (Hirsute Hippo)

Last updated: May 17,2024

1. Install "cpl-plugin-uves" package

Please follow the step by step instructions below to install cpl-plugin-uves on Ubuntu 21.04 (Hirsute Hippo)

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

2. Uninstall "cpl-plugin-uves" package

This guide let you learn how to uninstall cpl-plugin-uves on Ubuntu 21.04 (Hirsute Hippo):

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

3. Information about the cpl-plugin-uves package on Ubuntu 21.04 (Hirsute Hippo)

Package: cpl-plugin-uves
Architecture: amd64
Version: 6.1.3+dfsg-3
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: 3721
Depends: libc6 (>= 2.33), libcext0 (>= 5.3.1), libcfitsio9 (>= 3.480~), libcplcore26 (>= 6.4), libcpldfs26 (>= 6.0), libcpldrs26 (>= 6.4), libcplui26 (>= 6.4), libgomp1 (>= 4.9), 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-3_amd64.deb
Size: 1075684
MD5sum: b0186720d7614a34761b83fb008fc323
SHA1: ceac7a040a6a77594e63b2b7a77fb42905abdf2d
SHA256: 37e3b2682d1cffcce6df88fa6c3c67f789fc157deb0e1f1d049c7d502711e3fd
SHA512: 1dc510b6b6806932a6598b7291a33529e295808ff594df0ebfbbe4750995a1230d91f00ed295125bc44021637e36e0b0ba618bb4a64f44aba2867b05f1c78e0f
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