How to Install and Uninstall cpl-plugin-hawki Package on Ubuntu 16.04 LTS (Xenial Xerus)

Last updated: May 04,2024

1. Install "cpl-plugin-hawki" package

Here is a brief guide to show you how to install cpl-plugin-hawki on Ubuntu 16.04 LTS (Xenial Xerus)


    
        
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                sudo apt update
            
                    
    
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            $
        

        
            
                sudo apt install
            
                        
                cpl-plugin-hawki
            
                    
    
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2. Uninstall "cpl-plugin-hawki" package

This tutorial shows how to uninstall cpl-plugin-hawki on Ubuntu 16.04 LTS (Xenial Xerus):


    
        
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                sudo apt remove
            
                        
                cpl-plugin-hawki
            
                    
    
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                sudo apt autoclean && sudo apt autoremove
            
                    
    
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3. Information about the cpl-plugin-hawki package on Ubuntu 16.04 LTS (Xenial Xerus)

Package: cpl-plugin-hawki
Priority: optional
Section: universe/science
Installed-Size: 896
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astronomy Maintainers
Architecture: amd64
Version: 1.8.18+dfsg-5
Depends: libc6 (>= 2.14), libcplcore20 (>= 6.0), libcpldfs20 (>= 6.0), libcpldrs20 (>= 6.0), libcplui20 (>= 6.3), libgcc1 (>= 1:3.0), libgomp1 (>= 4.9), libgsl2, libstdc++6 (>= 4.1.1)
Recommends: esorex | python-cpl
Suggests: cpl-plugin-hawki-calib (= 1.8.18+dfsg-5), cpl-plugin-hawki-doc
Filename: pool/universe/c/cpl-plugin-hawki/cpl-plugin-hawki_1.8.18+dfsg-5_amd64.deb
Size: 199012
MD5sum: b01c49b7c03387d9f4feb6040374c806
SHA1: 3471e1b68664943242ad6077ade94a6dcd742ee6
SHA256: 318e3cdf027b1088e2bd10a59d696200ce37664d96e4ce2f5d0c6a0bdc7f1631
Description-en: ESO data reduction pipeline for HAWK-I
This is the data reduction pipeline for the HAWK-I instrument of the
Very Large Telescope (VLT) from the European Southern Observatory (ESO).
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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: 4bd8605f9cde93b47824d14c59741626
Multi-Arch: same
Homepage: http://www.eso.org/sci/software/pipelines/hawki
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Origin: Ubuntu