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

Last updated: November 07,2024

1. Install "cpl-plugin-muse" package

In this section, we are going to explain the necessary steps to install cpl-plugin-muse on Ubuntu 16.04 LTS (Xenial Xerus)


    
        
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                sudo apt update
            
                    
    
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                sudo apt install
            
                        
                cpl-plugin-muse
            
                    
    
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2. Uninstall "cpl-plugin-muse" package

In this section, we are going to explain the necessary steps to uninstall cpl-plugin-muse on Ubuntu 16.04 LTS (Xenial Xerus):


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

Package: cpl-plugin-muse
Priority: optional
Section: universe/science
Installed-Size: 1932
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astronomy Maintainers
Architecture: amd64
Version: 1.2.1+dfsg-2
Depends: libc6 (>= 2.14), libcplcore20 (>= 6.4), libcpldfs20 (>= 6.5), libcpldrs20 (>= 6.4), libcplui20 (>= 6.3), libgomp1 (>= 4.9)
Recommends: esorex | python-cpl
Suggests: cpl-plugin-muse-calib, cpl-plugin-muse-doc
Filename: pool/universe/c/cpl-plugin-muse/cpl-plugin-muse_1.2.1+dfsg-2_amd64.deb
Size: 431098
MD5sum: fafcdfd3a3ffa05e60b2ed59b9bd47e2
SHA1: 13cd59fe345ce2321693ce413f99a9a0b6e26eba
SHA256: 89c377f4cfb545fd22d9603e9af68ee4c5e737b7788b304eb5ca14074f065ca5
Description-en: 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: b152a7b24acf2ae5bc2716c812f83b3b
Multi-Arch: same
Homepage: http://www.eso.org/sci/software/pipelines/muse
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Origin: Ubuntu