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

Last updated: May 21,2024

1. Install "cpl-plugin-uves" package

In this section, we are going to explain the necessary steps to install cpl-plugin-uves on Ubuntu 20.10 (Groovy Gorilla)

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

2. Uninstall "cpl-plugin-uves" package

Please follow the instructions below to uninstall cpl-plugin-uves on Ubuntu 20.10 (Groovy Gorilla):

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

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

Package: cpl-plugin-uves
Architecture: amd64
Version: 6.1.3+dfsg-2build1
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: 3725
Depends: libc6 (>= 2.29), 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-2build1_amd64.deb
Size: 1075324
MD5sum: bdc61c3140b54e61770f252b87756a17
SHA1: 8e9663f40bce609d567cfd350a56ff4b73f4b772
SHA256: 4be0294dc371d8e36f2feaa7f51c7541ff82a1d4894780b3d231df24ed737d5e
SHA512: 4ecee3bc7d2fab99521014df0accb29536e9b90b95fe39aadcae4c6310696e2839f848f8f2bc9765f3cdaa0a5ad22bb91046068e4debbbd02f5ffa04837e5b04
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