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

Last updated: May 17,2024

1. Install "cpl-plugin-hawki" package

This tutorial shows how to install cpl-plugin-hawki on Ubuntu 21.04 (Hirsute Hippo)

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

2. Uninstall "cpl-plugin-hawki" package

Please follow the steps below to uninstall cpl-plugin-hawki on Ubuntu 21.04 (Hirsute Hippo):

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

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

Package: cpl-plugin-hawki
Architecture: amd64
Version: 2.4.8+dfsg-2
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: 1884
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 (>= 5)
Recommends: esorex | python3-cpl
Suggests: cpl-plugin-hawki-calib (= 2.4.8+dfsg-2), cpl-plugin-hawki-doc
Filename: pool/universe/c/cpl-plugin-hawki/cpl-plugin-hawki_2.4.8+dfsg-2_amd64.deb
Size: 442652
MD5sum: fd0a99fd87ea6d206d86366a3934351d
SHA1: 6a4ad52175327571a2111da32aaf8e76aae7ad74
SHA256: 41322cb2a22885e3d4a3acee92bf9d49a9295856773813722dce6a95c7c490d9
SHA512: 49164f1677d64a2e25a4a755b2dc9a6040235a32e379ee7fe7ce06d0bd9731a2bc8da205d1105a712f1a3866ede36797b27fd60aa982f1bc02e63f90f2edfd6a
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