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

Last updated: May 17,2024

1. Install "cpl-plugin-hawki" package

This tutorial shows how to install cpl-plugin-hawki on Ubuntu 20.10 (Groovy Gorilla)

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

2. Uninstall "cpl-plugin-hawki" package

Here is a brief guide to show you how to uninstall cpl-plugin-hawki on Ubuntu 20.10 (Groovy Gorilla):

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

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

Package: cpl-plugin-hawki
Architecture: amd64
Version: 2.4.8+dfsg-1
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: 1896
Depends: libc6 (>= 2.29), libcplcore26 (>= 6.3), libcpldfs26 (>= 6.0), libcpldrs26 (>= 6.4), libcplui26 (>= 6.4), libgcc-s1 (>= 3.0), libgomp1 (>= 4.9), libgsl25 (>= 2.6), libstdc++6 (>= 4.1.1)
Recommends: esorex | python3-cpl
Suggests: cpl-plugin-hawki-calib (= 2.4.8+dfsg-1), cpl-plugin-hawki-doc
Filename: pool/universe/c/cpl-plugin-hawki/cpl-plugin-hawki_2.4.8+dfsg-1_amd64.deb
Size: 444580
MD5sum: ee1cf1e506be1352efc2ad320a71ccbb
SHA1: fa1dc8d1f6611c17a9a9c0bc3858c859947087a9
SHA256: 1e51e963380e52e923dc2d3ae2bb12e025ef6c17568b11b57ca823b3ab853df1
SHA512: a7409ffb66ddeb79b3a01f00efee6438c48575918a3ca0511e37ccd80305a16cf5f3e151ed851c237b2818f37e2a12d099895c8f4c72f8996228e50327303f03
Homepage: https://www.eso.org/sci/software/pipelines/hawki
Description-en: ESO data reduction pipeline for the HAWK-I instrument
This is the data reduction pipeline for the HAWK-I instrument of the
Very Large Telescope (VLT) from the European Southern Observatory (ESO).
.
HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being
offered for the first time in Period 81. The instrument is cryogenic (120 K,
detectors at 80 K) and has a full reflective design. The light passes four
mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048
* 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky
corresponds to 169 μm on the detector).
Description-md5: b5fdefd451ec59ef97df02d8d7d3b708