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

Last updated: September 20,2024

1. Install "cpl-plugin-uves" package

Please follow the guidance below to install cpl-plugin-uves on Kali Linux


    
        
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                sudo apt update
            
                    
    
    Copied


    
        
            $
        

        
            
                sudo apt install
            
                        
                cpl-plugin-uves
            
                    
    
    Copied

2. Uninstall "cpl-plugin-uves" package

Please follow the instructions below to uninstall cpl-plugin-uves on Kali Linux:


    
        
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                sudo apt remove
            
                        
                cpl-plugin-uves
            
                    
    
    Copied


    
        
            $
        

        
            
                sudo apt autoclean && sudo apt autoremove
            
                    
    
    Copied

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

Package: cpl-plugin-uves
Source: cpl-plugin-uves (6.1.8+dfsg-2)
Version: 6.1.8+dfsg-2+b1
Installed-Size: 3723
Maintainer: Debian Astronomy Maintainers
Architecture: amd64
Depends: libc6 (>= 2.35), libcext0 (>= 5.3.1), libcfitsio10 (>= 4.2.0~), libcplcore26 (>= 6.4), libcpldfs26 (>= 6.0), libcpldrs26 (>= 6.4), libcplui26 (>= 6.4), libgomp1 (>= 4.9), libgsl27 (>= 2.7.1), libqfits0
Recommends: esorex | python3-cpl
Suggests: cpl-plugin-uves-calib, cpl-plugin-uves-doc
Size: 1103052
SHA256: 6e941cad663b2ea03e652784e20cd935c87f616c80364b47f92994448115f5ed
SHA1: e2775924ce9d3822f5151e596362029d712d66ec
MD5sum: be4064af382d97ee0c5bfecd95701c19
Description: ESO data reduction pipeline for the UVES instrument
This is the data reduction pipeline for the UVES instrument of the Very
Large Telescope (VLT) from the European Southern Observatory (ESO).
.
UVES is a cross-dispersed echelle spectrograph designed to operate with
high efficiency from the atmospheric cut-off at 300 nm to the long
wavelength limit of the CCD detectors (about 1100 nm). The light beam
from the telescope is split in two arms (UV to Blue, and Visual to Red)
within the instrument. The two arms can be operated separately, or in
parallel via a dichroic beam splitter. The resolving power is about
40,000 when a 1-arcsec slit is used. The maximum (two-pixel) resolution
is 80,000 or 110,000 in the Blue- and the Red Arm, respectively.
Description-md5:
Multi-Arch: same
Homepage: https://www.eso.org/sci/software/pipelines/uves
Section: science
Priority: optional
Filename: pool/main/c/cpl-plugin-uves/cpl-plugin-uves_6.1.8+dfsg-2+b1_amd64.deb