How to Install and Uninstall cpl-plugin-hawki Package on Kali Linux

Last updated: May 21,2024

1. Install "cpl-plugin-hawki" package

Please follow the step by step instructions below to install cpl-plugin-hawki on Kali Linux


    
        
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                sudo apt update
            
                    
    
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            $
        

        
            
                sudo apt install
            
                        
                cpl-plugin-hawki
            
                    
    
    Copied

2. Uninstall "cpl-plugin-hawki" package

This is a short guide on how to uninstall cpl-plugin-hawki on Kali Linux:


    
        
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                sudo apt remove
            
                        
                cpl-plugin-hawki
            
                    
    
    Copied


    
        
            $
        

        
            
                sudo apt autoclean && sudo apt autoremove
            
                    
    
    Copied

3. Information about the cpl-plugin-hawki package on Kali Linux

Package: cpl-plugin-hawki
Source: cpl-plugin-hawki (2.4.11+dfsg-1)
Version: 2.4.11+dfsg-1+b1
Installed-Size: 1842
Maintainer: Debian Astronomy Maintainers
Architecture: amd64
Depends: libc6 (>= 2.29), libcplcore26 (>= 6.3), libcpldfs26 (>= 6.0), libcpldrs26 (>= 6.4), libcplui26 (>= 6.4), libgcc-s1 (>= 3.0), libgomp1 (>= 4.9), libgsl27 (>= 2.7.1), libstdc++6 (>= 5)
Recommends: esorex | python3-cpl
Suggests: cpl-plugin-hawki-calib (= 2.4.11+dfsg-1+b1), cpl-plugin-hawki-doc
Size: 493028
SHA256: a5ef913619d8b828dbad1339784f77aacd7d2529f8b54b1b3e72573f4da86315
SHA1: 7ce50e8f631c0ff295d41a89c93cafb28e40e29c
MD5sum: 0180fbb9388b9036b16d41fd139369de
Description: 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).
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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:
Multi-Arch: same
Homepage: https://www.eso.org/sci/software/pipelines/hawki
Section: science
Priority: optional
Filename: pool/main/c/cpl-plugin-hawki/cpl-plugin-hawki_2.4.11+dfsg-1+b1_amd64.deb