<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Cosmic Voids |</title><link>https://tommasoronconi.github.io/tags/cosmic-voids/</link><atom:link href="https://tommasoronconi.github.io/tags/cosmic-voids/index.xml" rel="self" type="application/rss+xml"/><description>Cosmic Voids</description><generator>HugoBlox Kit (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Wed, 01 Nov 2017 00:00:00 +0000</lastBuildDate><image><url>https://tommasoronconi.github.io/media/icon.svg</url><title>Cosmic Voids</title><link>https://tommasoronconi.github.io/tags/cosmic-voids/</link></image><item><title>CosmoBolognaLib</title><link>https://tommasoronconi.github.io/software/cosmobolognalib/</link><pubDate>Wed, 01 Nov 2017 00:00:00 +0000</pubDate><guid>https://tommasoronconi.github.io/software/cosmobolognalib/</guid><description>&lt;p&gt;&lt;strong&gt;Role:&lt;/strong&gt; contributor — void size function modelling and void-catalogue cleaning.
&lt;strong&gt;Stack:&lt;/strong&gt; C++ libraries with a SWIG-generated Python wrapper.
&lt;strong&gt;Author &amp;amp; maintainer:&lt;/strong&gt; Federico Marulli (Università di Bologna).&lt;/p&gt;
&lt;p&gt;CosmoBolognaLib (CBL) is a living project that provides a common numerical environment for
cosmological investigations of the large-scale structure of the Universe. Its focus is
handling astronomical catalogues — real and simulated — measuring one-, two- and three-point
statistics in configuration space, and running cosmological analyses.&lt;/p&gt;
&lt;p&gt;My contribution is the set of tools for cosmic voids: the algorithm that redefines void
ridges and therefore their radii, together with the model for the void size function. The
cleaning procedure takes a void catalogue produced by a void finder and returns a catalogue
of non-overlapping spheres, each embedding a fixed density contrast in the tracer density
field — which is what makes the measured size function comparable with theoretical
predictions. These functions were released in CBL v3.2 and are credited in the library&amp;rsquo;s
changelog to Ronconi &amp;amp; Marulli (2017).&lt;/p&gt;
&lt;p&gt;The tooling underpins the void work described in my
, and was subsequently adopted in Key
Projects within the Euclid Collaboration to forecast the cosmological constraining power of
void statistics.&lt;/p&gt;
&lt;p&gt;The void tools are presented in &lt;em&gt;Astronomy &amp;amp; Astrophysics&lt;/em&gt; 607, A24 (2017) — see
. The library itself is described in Marulli,
Veropalumbo &amp;amp; Moresco (2016).&lt;/p&gt;</description></item></channel></rss>