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

Last updated: May 09,2024

1. Install "cpl-plugin-visir" package

In this section, we are going to explain the necessary steps to install cpl-plugin-visir on Kali Linux


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

2. Uninstall "cpl-plugin-visir" package

Please follow the guidelines below to uninstall cpl-plugin-visir on Kali Linux:


    
        
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                sudo apt remove
            
                        
                cpl-plugin-visir
            
                    
    
    Copied


    
        
            $
        

        
            
                sudo apt autoclean && sudo apt autoremove
            
                    
    
    Copied

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

Package: cpl-plugin-visir
Source: cpl-plugin-visir (4.4.2+dfsg-1)
Version: 4.4.2+dfsg-1+b1
Installed-Size: 2493
Maintainer: Debian Astronomy Team
Architecture: amd64
Depends: libc6 (>= 2.35), libcext0 (>= 5.3.1), libcplcore26 (>= 6.4), libcpldfs26 (>= 6.0), libcpldrs26 (>= 6.4), libcplui26 (>= 6.4), libgomp1 (>= 4.9), libgsl27 (>= 2.7.1), swarp
Recommends: esorex | python3-cpl
Suggests: cpl-plugin-visir-calib, cpl-plugin-visir-doc
Size: 669464
SHA256: c0e10ddb652417a86f69e8f4b6d54379d8f15ff8001fd378412178ed22c9149e
SHA1: ec3942f59fd7a79f5c7d90c9702725eaa565b88e
MD5sum: c7ff2f28d20d6d0a04060f024d847a95
Description: 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:
Multi-Arch: same
Homepage: https://www.eso.org/sci/software/pipelines/visir
Section: science
Priority: optional
Filename: pool/main/c/cpl-plugin-visir/cpl-plugin-visir_4.4.2+dfsg-1+b1_amd64.deb