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

Last updated: May 03,2024

1. Install "cpl-plugin-uves" package

Please follow the step by step instructions below to install cpl-plugin-uves on Ubuntu 16.04 LTS (Xenial Xerus)


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

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


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

Package: cpl-plugin-uves
Priority: optional
Section: universe/science
Installed-Size: 3081
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astronomy Maintainers
Architecture: amd64
Version: 5.5.7+dfsg-1
Depends: libc6 (>= 2.14), libcext0 (>= 5.3.1), libcfitsio2 (>= 3.370), libcplcore20 (>= 6.3), libcpldfs20 (>= 6.0), libcpldrs20 (>= 6.0), libcplui20 (>= 6.4), libqfits0
Recommends: esorex | python-cpl
Suggests: cpl-plugin-uves-calib, cpl-plugin-uves-doc
Filename: pool/universe/c/cpl-plugin-uves/cpl-plugin-uves_5.5.7+dfsg-1_amd64.deb
Size: 911524
MD5sum: e2d92be067742a6bf683e91d406d363f
SHA1: 4a412780a23a6b2f55c2548a83859db15eac5c61
SHA256: fdc6f28959e6c0b0b5fc3a60088c278d9d50d60be555fd1da600239d53085f75
Description-en: ESO data reduction pipeline for UVES
This is the data reduction pipeline for the UVES instrument of the Very
Large Telescope (VLT) from the European Southern Observatory (ESO).
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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: 7429ead2289ec4c4041aa4aef3ee13d7
Multi-Arch: same
Homepage: http://www.eso.org/sci/software/pipelines/uves
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Origin: Ubuntu