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<html>
<head>
<title>NUPYCEE</title>
</head>
<body bgcolor=white>
<table border="0" cellpadding="10">
<tr>
<td>
<h1>Welcome to the NUPYCEE website</h1>
</td>
</tr>
</table>
<p> NUPYCEE is a <b>open-source</b> chemical evolution platform of the <a href="http://nugridstars.org">NuGrid collaboration</a>.
The user can choose between the Stellar Yields for galactic modeling applications (<b>SYGMA</b>) module and the One-zone model for the evolution of galaxies (<b>OMEGA</b>) module.
</p>
<hr>
<h2> SYGMA web user interface </h2>
<p>
The Stellar Yields for galactic modeling applications (<b>SYGMA</b>) module allows to follow the ejecta of of simple stellar populations in a closed-box mode.
</p>
<p>We provide an online interface where tables of the evolution of the ejecta of SSP's can be downloaded.
Access the interface <a href="http://206.12.59.19/cgi-bin/canfarSessionLauncher.py" target="_blank">here</a>.
Start the ipython notebook SYGMA.ipynb with a click. Then you can create the SYGMA interface by clicking in the first field and
press shift+enter. For a introduction to the interface have a look <a href="DOC_Interfaces/sygma_doc.html">here</a>.
</p>
<h4> Notes: </h4>
<p>
Stellar yields of AGB and massive stars are calculated with the same nuclear physics and are provided by the NuGrid collaboration.
The interface is hosted by NuGrid's WENDI platform.
</p>
<hr>
<h2> Online User guides </h2>
<p>
As a introduction to the SYGMA and OMEGA code as well as STELLAB module we provide different
interactive online user guides.
One can access the web interface <a href="http://206.12.59.19/cgi-bin/canfarSessionLauncher.py" target="_blank">here</a>
and choose from the following guides:
</p>
<ol>
<li type="circle">SYGMA_Userguide</li>
<li type="circle">OMEGA_Userguide</li>
<li type="circle">STELLAB_Userguide</li>
</ol>
<p>
Within each guide the user can execute commands in the same manner as in
in a local downloaded version with a few exceptions.
</p>
<hr>
<h2> Download code </h2>
All NUPYCEE is publicly available on github.
To download the code git is required on your system.
First create a directory, for example NUPYCEE, and navigate in it:
<div class="highlight">
<pre>
<code class="language-text" data-lang="text">mkdir NuPyCEE</code>
<code class="language-text" data-lang="text">cd NuPyCEE</code>
</pre>
</div>
Now download a copy with
<div class="highlight"></div>
<pre>
<code class="language-text" data-lang="text">git clone https://github.com/NuGrid/NuPyCEE.git .</code>
</pre>
</div>
<p>The repository can be found <a href="https://github.com/NuGrid/NuPyCEE">here</a>.</p>
<hr>
<h2> Running SYGMA and OMEGA locally </h2>
The ipython environment with numpy and matplotlib are required.
A installation of NUPYCEE is not necessary. Instead, you can access the tools through the ipython interactive interface.
To run SYGMA and OMEGA have a look at the tutorials in the online documentations (links below) and
the <a href="DOC/nupycee-chapter.pdf">DOC</a> directory of NUPYCEE .</p>
<p>The online documentation for SYGMA can be found <a href="http://nupycee.bitbucket.org/SPHINX/build/html/sygma.html">here</a> and for OMEGA <a href="http://nupycee.bitbucket.org/SPHINX/build/html/omega.html">here</a>.</p>
Detailed explanation of physics and input parameter for OMEGA are found on the WENDI platform in
OMEGA_Userguide.ipynb <a href="http://206.12.59.19/cgi-bin/canfarSessionLauncher.py" target="_blank">here</a>.
<hr>
<hr>
© Christian Ritter, Benoit Côté, critter[a]uvic.ca, 2016
</body>
</html>