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<div class="section" id="changelog">
<span id="id1"></span><h1>Changelog<a class="headerlink" href="#changelog" title="Permalink to this headline">¶</a></h1>
<div class="admonition-todo admonition" id="id4">
<p class="admonition-title">Todo</p>
<ul class="simple">
<li><p>(!) allow to abort the continuum fitting with CTRL-C</p></li>
<li><p><cite>run_crude_snr_maps</cite>: compute proper S/N for bright stars (not <>/std !)</p></li>
<li><p>enable minorticks in colorbars (see astropy bug <a class="reference external" href="https://github.com/astropy/astropy/issues/8126">[8126]</a>)</p></li>
<li><p>set the color of NaN pixels in plots … (see astropy bug <a class="reference external" href="https://github.com/astropy/astropy/issues/8165">[8165]</a>)</p></li>
<li><p>when drawing contours in <cite>run_skysub()</cite>, show the actual pixel edges</p></li>
<li><p>allow for an automated selection of the sky areas -> requires a better snr estimate ?</p></li>
<li><p>(?) use <cite>config.parser</cite> to feed in the parameters, instead of YAML</p></li>
<li><p>(?) add scalebar to plots … tricky: what if pix scale not uniform, North not up, etc …</p></li>
</ul>
</div>
<p>v2019.08.3: F.P.A. Vogt
- continued with pylint a bit more … re-ouch …
- added PyYAML to the list of required packages in <cite>setup.py</cite>
- fixed <cite>MANIFEST.in</cite> to include the .yaml setup files!</p>
<p>v2019.08.2: F.P.A. Vogt
- improved the WCS function, to minimize memory use in crowded fields.
- full restructuration of the high-level operation of the code, with proper entry point, via a new <cite>run()</cite> function
- split the WCS correction function, so that it can also be used (potentially) as a stand-alone tool for 2D images.
- started using pylint … ouch!
- worked on the plotting routines, to make them more robust and uniform.</p>
<p>v2019.08.1: F.P.A Vogt
- improved the WCS adjustment step, in case the reference pixel is not in the middle of the image (found by J. Suherli with OCam data).
- added automatic inclusion of code version in setup.py
- added a proper <code class="docutils literal notranslate"><span class="pre">brutifus</span></code> entry point from the console.</p>
<p>v2019.07.1: F.P.A. Vogt
- added courtesy function to create the execution files, via <cite>python -m brutifus –setup</cite>.
- added a proper entry point, so this can be run as <cite>brutifus –setup</cite>.
- carry over the full original headers when adjusting the WCS values.
- fixed a bug in the WCS adjustment function that led to an error of 0.5 pixel for odd array sizes</p>
<dl class="simple">
<dt>v2019.02.3: F.P.A. Vogt</dt><dd><ul class="simple">
<li><p>following the suggestion from Nick Whyborn, use image convolution to find the best
spatial shift required to anchor the cube WCS on Gaia.</p></li>
<li><p>removed all references to aplpy</p></li>
</ul>
</dd>
<dt>v2019.02.2: F.P.A. Vogt</dt><dd><ul class="simple">
<li><p>added photutils to the list of required packages</p></li>
<li><p>fixed all docstrings</p></li>
<li><p>cleaned up code of all old brutus bits not (yet) ported to brutifus.</p></li>
<li><p>started working on documentation</p></li>
<li><p>first public release!</p></li>
</ul>
</dd>
<dt>v2019.02.1: F.P.A. Vogt</dt><dd><ul class="simple">
<li><p>added run_BWplot step</p></li>
<li><p>aded WCS correction step</p></li>
<li><p>worked a bit on refactoring the docstrings</p></li>
</ul>
</dd>
<dt>v2019.01.1: F.P.A. Vogt</dt><dd><ul class="simple">
<li><p>revived the reddening module</p></li>
</ul>
</dd>
<dt>v2018.11.1: F.P.A. Vogt</dt><dd><ul class="simple">
<li><p>added the ‘raw_cube’ name to fn_list for easy access</p></li>
</ul>
</dd>
<dt>v2018.11.0: F.P.A. Vogt</dt><dd><ul class="simple">
<li><p>ported brutus to python 3, renamed it to brutifus (available pip name)</p></li>
<li><p>removed ppxf from brutifus (focus on SNRs for now)</p></li>
<li><p>removed pyqz from brutifus (outdated)</p></li>
<li><p>added sky-subtraction step</p></li>
<li><p>initial upload to Github, initial upload to pip</p></li>
</ul>
</dd>
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