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<!DOCTYPE html>
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<div class="section" id="brutifus-release">
<h1>brutifus 2019.08.3<a class="headerlink" href="#brutifus-release" title="Permalink to this headline">¶</a></h1>
<p><a class="reference external" href="https://pypi.python.org/pypi/brutifus/"><img alt="pypi" src="https://img.shields.io/pypi/v/brutifus.svg?colorB=<brightgreen>" /></a> <a class="reference external" href="https://zenodo.org/badge/latestdoi/157203434"><img alt="DOI_latest" src="https://zenodo.org/badge/157203434.svg" /></a> <a class="reference external" href="http://ascl.net/1903.004"><img alt="ascl" src="https://img.shields.io/badge/ascl-1903.004-blue.svg?colorB=262255" /></a> <a class="reference external" href="http://www.astropy.org/"><img alt="astropy" src="http://img.shields.io/badge/powered%20by-AstroPy-orange.svg?style=flat" /></a> <a class="reference external" href="https://github.com/fpavogt/brutifus"><img alt="last-commit" src="https://img.shields.io/github/last-commit/fpavogt/brutifus.svg?colorB=e6c000" /></a></p>
<p>brutifus is a set of Python routines designed to post-process datacubes from Integral Field
Spectrographs, and in particular MUSE and WiFeS. The spirit of brutifus is to deal with
<em>generic</em> post-processing tasks with as little interactions as possible.</p>
<p>So far, brutifus allows to:</p>
<blockquote>
<div><ul class="simple">
<li><p><strong>correct a cube WCS solution</strong> using Gaia,</p></li>
<li><p><strong>generate B&W and RGB images from the cube</strong>,</p></li>
<li><p><strong>correct for the galactic reddening along the line of sight</strong>,</p></li>
<li><p><strong>fit the stellar/nebular continuum</strong> using the non-parametric Locally Weighted
Scatterplot Smoothing (LOWESS) technique,</p></li>
<li><p><strong>perform an ad-hoc sky-subtraction</strong> if required.</p></li>
</ul>
</div></blockquote>
<p>brutifus is modular: <cite>execution</cite> files allow the user to specify which recipe is to be
executed, and in which order. Wherever feasible/beneficial, brutifus routines can use up
to <code class="docutils literal notranslate"><span class="pre">ny</span></code> cpus at once (where <code class="docutils literal notranslate"><span class="pre">nx*ny</span></code> is the number of spaxels in the datacube;
<code class="docutils literal notranslate"><span class="pre">ny~300</span></code> for a MUSE cube) to speed up the processing of large datasets.</p>
<div class="admonition note">
<p class="admonition-title">Note</p>
<p>brutifus is very much a work in progress. Modules and recipes will get added as
the need arises. The code is released publicly because I believe in an open
Science policy.</p>
<p>You’re welcome to try it out … so long as you remember that the code comes with
no warranty!</p>
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<h2>Contents<a class="headerlink" href="#contents" title="Permalink to this headline">¶</a></h2>
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<h3>Copyright notice<a class="headerlink" href="#copyright-notice" title="Permalink to this headline">¶</a></h3>
<p>This file is part of the brutifus Python module.
The brutifus Python module is free software: you can redistribute it and/or modify it under
the terms of the GNU General Public License as published by the Free Software Foundation,
version 3 of the License.</p>
<p>The brutifus Python module is distributed in the hope that it will be useful, but without any
warranty; without even the implied warranty of merchantability or fitness for a particular
purpose. See the GNU General Public License for more details.</p>
<p>You should have received a copy of the GNU General Public License along with the brutifus
Python module. If not, see <a class="reference external" href="http://www.gnu.org/licenses/">http://www.gnu.org/licenses/</a> .</p>
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