How to Install and Uninstall eso-pipelines Package on Ubuntu 16.04 LTS (Xenial Xerus)
Last updated: December 28,2024
1. Install "eso-pipelines" package
Please follow the steps below to install eso-pipelines on Ubuntu 16.04 LTS (Xenial Xerus)
$
sudo apt update
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$
sudo apt install
eso-pipelines
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2. Uninstall "eso-pipelines" package
Here is a brief guide to show you how to uninstall eso-pipelines on Ubuntu 16.04 LTS (Xenial Xerus):
$
sudo apt remove
eso-pipelines
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$
sudo apt autoclean && sudo apt autoremove
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3. Information about the eso-pipelines package on Ubuntu 16.04 LTS (Xenial Xerus)
Package: eso-pipelines
Priority: optional
Section: universe/science
Installed-Size: 11
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astronomy Team
Architecture: all
Version: 1.0
Recommends: cpl-plugin-amber, cpl-plugin-fors, cpl-plugin-giraf, cpl-plugin-hawki, cpl-plugin-kmos, cpl-plugin-muse, cpl-plugin-naco, cpl-plugin-sinfo, cpl-plugin-uves, cpl-plugin-vimos, cpl-plugin-visir, cpl-plugin-xshoo, esorex, python-cpl, python3-cpl
Filename: pool/universe/e/eso-pipelines/eso-pipelines_1.0_all.deb
Size: 2044
MD5sum: 08d5336777b0d51aad6ae2324380de35
SHA1: a573c6ed78418b1d347f5536274b289a82783a36
SHA256: 88aa2f6a60530b2412c3836df9ab09aad55498a6ca039c0476af9f3848568a5d
Description-en: ESO VLT Instrument pipeline collection
In collaboration with the various instrument consortia, the Pipeline Systems
Department has undertaken to implement data reduction pipelines for the most
commonly used VLT/VLTI instrument modes. These data reduction pipelines have
three main purposes:
.
* Data quality control: Pipelines are used to produce the quantitative
information necessary to monitor instrument performance.
.
* Master calibration product creation: pipelines are used to produce master
calibration products (e.g. combined bias frames, super-flats, wavelength
dispersion solutions).
.
* Science product creation: using pipeline-generated master calibration
products, science products are produced for supported instrument modes
(e.g. combined ISAAC jitter stacks; bias-corrected, flat-fielded FORS
images, wavelength-calibrated UVES spectra). The accuracy of the science
products can be limited both by the quality of the available master
calibration products and by the algorithmic implementation of the
pipelines themselves. In particular, adopted reduction strategies may not
be suitable for all scientific goals.
.
This metapackage will install all ESO VLT pipelines along with the
environments needed to run them (esorex, python-cpl).
Description-md5: 41deaa80391e58098eb06b75e7f3956b
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Origin: Ubuntu
Priority: optional
Section: universe/science
Installed-Size: 11
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astronomy Team
Architecture: all
Version: 1.0
Recommends: cpl-plugin-amber, cpl-plugin-fors, cpl-plugin-giraf, cpl-plugin-hawki, cpl-plugin-kmos, cpl-plugin-muse, cpl-plugin-naco, cpl-plugin-sinfo, cpl-plugin-uves, cpl-plugin-vimos, cpl-plugin-visir, cpl-plugin-xshoo, esorex, python-cpl, python3-cpl
Filename: pool/universe/e/eso-pipelines/eso-pipelines_1.0_all.deb
Size: 2044
MD5sum: 08d5336777b0d51aad6ae2324380de35
SHA1: a573c6ed78418b1d347f5536274b289a82783a36
SHA256: 88aa2f6a60530b2412c3836df9ab09aad55498a6ca039c0476af9f3848568a5d
Description-en: ESO VLT Instrument pipeline collection
In collaboration with the various instrument consortia, the Pipeline Systems
Department has undertaken to implement data reduction pipelines for the most
commonly used VLT/VLTI instrument modes. These data reduction pipelines have
three main purposes:
.
* Data quality control: Pipelines are used to produce the quantitative
information necessary to monitor instrument performance.
.
* Master calibration product creation: pipelines are used to produce master
calibration products (e.g. combined bias frames, super-flats, wavelength
dispersion solutions).
.
* Science product creation: using pipeline-generated master calibration
products, science products are produced for supported instrument modes
(e.g. combined ISAAC jitter stacks; bias-corrected, flat-fielded FORS
images, wavelength-calibrated UVES spectra). The accuracy of the science
products can be limited both by the quality of the available master
calibration products and by the algorithmic implementation of the
pipelines themselves. In particular, adopted reduction strategies may not
be suitable for all scientific goals.
.
This metapackage will install all ESO VLT pipelines along with the
environments needed to run them (esorex, python-cpl).
Description-md5: 41deaa80391e58098eb06b75e7f3956b
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Origin: Ubuntu