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

Last updated: May 09,2024

1. Install "cpl-plugin-visir" package

Please follow the steps below to install cpl-plugin-visir on Ubuntu 16.04 LTS (Xenial Xerus)


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

This is a short guide on how to uninstall cpl-plugin-visir on Ubuntu 16.04 LTS (Xenial Xerus):


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

Package: cpl-plugin-visir
Priority: optional
Section: universe/science
Installed-Size: 1825
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astronomy Team
Architecture: amd64
Version: 4.1.0+dfsg-2
Depends: libc6 (>= 2.14), libcext0 (>= 5.3.1), libcplcore20 (>= 6.4), libcpldfs20 (>= 6.0), libcpldrs20 (>= 6.0), libcplui20 (>= 6.4), libgomp1 (>= 4.9), swarp
Recommends: esorex | python-cpl
Suggests: cpl-plugin-visir-calib, cpl-plugin-visir-doc
Filename: pool/universe/c/cpl-plugin-visir/cpl-plugin-visir_4.1.0+dfsg-2_amd64.deb
Size: 403742
MD5sum: 2b9b3dd10ccb0e0c1c970c9a9b12d0eb
SHA1: c07bd31976a2032da1a704270efd2b31d9271e64
SHA256: 6f587a96d953ce25216eac33d46777eb0a006fd2343164e53c51ee325d30a52e
Description-en: ESO data reduction pipeline for the VISIR instrument
This is the data reduction pipeline for the Visir instrument of the
Very Large Telescope (VLT) from the European Southern Observatory (ESO).
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The VLT spectrometer and imager for the mid-infrared (VISIR) was built by
CEA/DAPNIA/SAP and NFRA/ASTRON, and is located at the Cassegrain focus of
UT3. It provides diffraction-limited imaging at high sensitivity in the two
mid infrared (MIR) atmospheric windows: the N band between 8 to 13μm and the Q
band between 16.5 and 24.5μm, respectively. In addition, it features a
long-slitspectrometer with a range of spectral resolutions between 150 and
30000.
Description-md5: 336cd6b35449170af84b52cb432faf84
Multi-Arch: same
Homepage: http://www.eso.org/sci/software/pipelines/visir
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Origin: Ubuntu