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<html>
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<title>Code page of Julien Lesgourgues</title>
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<a href="index.html">home</a>
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<a href="presentation.html">presentation</a>
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<a href="courses.html">courses</a>
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codes
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<a href="events.html">events</a>
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<a href="outreach.html">outreach</a>
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<img src="images/v50.gif">
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<h1 align=center>Codes</h1>
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<img src="images/usine_rond.gif">
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<h3><a href="http://class-code.net" target="new">CLASS</a>: the Cosmic Linear Anisotropy Solving System</h3>
<ul>
<li> visit the CLASS web page <a href="http://class-code.net" target="new">http://class-code.net</a></li>
<li> or directly clone the <a href="https://github.com/lesgourg/class_public" target="new">class_public</a> git repository, and look at its <a href="https://github.com/lesgourg/class_public/wiki" target="new">wiki</a>
<li> courses and lecture notes on <a href="http://class-code.net" target="new">CLASS</a> are available on my <a href="courses.html">course page</a>
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<h3>Beyond <a href="http://class-code.net" target="new">CLASS</a>:</h3>
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<li> in <a href="http://www.thphys.uni-heidelberg.de/~zumalacarregui/hi_class.html" target="new">hi_class</a>, Miguel Zumalacarregui, Emilio Bellino and Ignacy Sawicki have extended <a href="http://class-code.net" target="new">CLASS</a> to a wide class of modified gravity models (Horndeski theories)
<li> in <a href="http://www.thphys.uni-heidelberg.de/~zumalacarregui/hi_class.html" target="new">SONG</a>, Guido Pettinari, Christian Fidler and Thomas Tram have generalised <a href="http://class-code.net" target="new">CLASS</a> to second order in perturbation theory
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<h3><a href="http://baudren.github.io/montepython.html" target="new">Monte Python</a>: a Monte Carlo code in Python for cosmological parameter inference</h3>
<ul>
<li> visit the Monte Python web page <a href="http://baudren.github.io/montepython.html" target="new">http://baudren.github.io/montepython.html</a></li>
<li> or directly clone the <a href="https://github.com/brinckmann/montepython_public" target="new">montepython_public</a> git repository, and look at its <a href="https://github.com/baudren/montepython_public/wiki" target="new">wiki</a>
<li> courses and lecture notes on <a href="http://baudren.github.io/montepython.html" target="new">Monte Python</a> are available on my <a href="courses.html">course page</a>
</ul>
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<h3>(Old) patches for <a href="http://camb.info/" target="new">CAMB</a> and <a href="http://cosmologist.info/cosmomc/" target="new">CosmoMC</a></h3>
<ul>
<li> <a href="http://lpsc.in2p3.fr/perotto/" target="new">FUTURCMB</a>: mock CMB data generator and parameter forecast modules <em> (including CMB lensing extraction) </em>. <br> For details, see "Probing cosmological parameters with the CMB: Forecasts from full Monte Carlo simulations" by Laurence Perotto, Julien Lesgourgues, Steen Hannestad, Huitzu Tu, Yvonne Y.Y. Wong, JCAP 0610 (2006) 013 <a href="http://arxiv.org/pdf/astro-ph/0606227" target="new">[astro-ph/0606227]</a>. The raw chains used in this paper can be <a href="codes/chains_0606227.html" target="new">downloaded here</a>.</li><br>
<li> <a href="https://www.wesselvalkenburg.nl//software/index.php?page=inflationh/" target="new">Inflation module</a> v2 (for computing numerically the scalar/tensor primordial spectra given a function H(phi) or V(phi), and for reconstructing the likelihood of the parameters of these functions from the data). <br> For details, see " What do WMAP and SDSS really tell about inflation?" by Julien Lesgourgues, Alexei A. Starobinsky, Wessel Valkenburg, JCAP01(2008)010 <a href="http://arxiv.org/pdf/0710.1630" target="new">[arXiv:0710.1630]</a>. Note that this module has also been translated and absorbed in the <tt>primordial</tt> module of <a href="http://class-code.net" target="new">CLASS</a>, with further options.</li><br>
<li> <a href="http://www.astro.caltech.edu/~rjm/cosmos/cosmomc/" target="new">3D Weak Lensing module</a> (for computing numerically the weak lensing angular correlation functions in various redhsift bins, and comparing with 2007 data from the HST <a href="http://arxiv.org/pdf/astro-ph/0701480" target="new">COSMOS</a> project). <br> For details, see "A Combined analysis of Lyman-alpha forest, 3D Weak Lensing and WMAP year three data" by Julien Lesgourgues, Matteo Viel, Martin G. Haehnelt, Richard Massey (Caltech), JCAP 0711:008,2007 <a href="http://arxiv.org/pdf/0705.0533" target="new">[arXiv:0705.0533]</a>. Note that this module has been reused in various weak lensing likelihoods which are part of the <a href="http://baudren.github.io/montepython.html" target="new">Monte Python</a> and <a href="http://cosmologist.info/cosmomc/" target="new">CosmoMC</a> packages. </li>
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Last update on the 17.09.2018. Back to <a href="index.html">home</a> page.
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