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

Last updated: November 22,2024

1. Install "cpl-plugin-muse" package

Learn how to install cpl-plugin-muse on Kali Linux


    
        
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                sudo apt update
            
                    
    
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                sudo apt install
            
                        
                cpl-plugin-muse
            
                    
    
    Copied

2. Uninstall "cpl-plugin-muse" package

Learn how to uninstall cpl-plugin-muse on Kali Linux:


    
        
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                sudo apt remove
            
                        
                cpl-plugin-muse
            
                    
    
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            $
        

        
            
                sudo apt autoclean && sudo apt autoremove
            
                    
    
    Copied

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

Package: cpl-plugin-muse
Source: cpl-plugin-muse (2.8.7+dfsg-3)
Version: 2.8.7+dfsg-3+b1
Installed-Size: 14592
Maintainer: Debian Astro Team
Architecture: amd64
Depends: libc6 (>= 2.35), libcext0 (>= 5.3.1), libcplcore26 (>= 7.2.2), libcpldfs26 (>= 6.5), libcpldrs26 (>= 6.4), libcplui26 (>= 6.3), libgomp1 (>= 4.9), libgsl27 (>= 2.7.1)
Recommends: esorex | python3-cpl
Suggests: cpl-plugin-muse-calib, cpl-plugin-muse-doc
Size: 1642352
SHA256: 8d961b72c9ff8362d6eb6452717dca5fc3a9c0517259dee994a8920983272ebf
SHA1: 24c69c42ed11d6d20e093ae96a55961a75796718
MD5sum: 0ef50ff4ce8cf6048d247dc3c1d31700
Description: ESO data reduction pipeline for the MUSE instrument
This is the data reduction pipeline for the Muse instrument of the
Very Large Telescope (VLT) from the European Southern Observatory (ESO).
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MUSE, the Multi-Unit Spectroscopic Explorer, is an Integral Field
Spectrograph located at the Nasmyth B focus of Yepun, the VLT UT4
telescope. It has a modular structure composed of 24 identical IFU modules
that together sample, in Wide Field Mode (WFM), a near-contiguous 1 squared
arcmin field of view. Spectrally the instrument samples almost the full
optical domain with a mean resolution of 3000. Spatially, the instrument
samples the sky with 0.2 arcseconds spatial pixels in the currently offered
Wide Field Mode with natural seeing (WFM-noAO).
Description-md5:
Multi-Arch: same
Homepage: https://www.eso.org/sci/software/pipelines/muse
Section: science
Priority: optional
Filename: pool/main/c/cpl-plugin-muse/cpl-plugin-muse_2.8.7+dfsg-3+b1_amd64.deb