<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Large-Scale Structure of the Universe; Cosmic Shear; Emulators; | Giovanni Aricò's website</title><link>https://garico92.github.io/website/tags/large-scale-structure-of-the-universe-cosmic-shear-emulators/</link><atom:link href="https://garico92.github.io/website/tags/large-scale-structure-of-the-universe-cosmic-shear-emulators/index.xml" rel="self" type="application/rss+xml"/><description>Large-Scale Structure of the Universe; Cosmic Shear; Emulators;</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Mon, 07 Aug 2023 00:00:00 +0000</lastBuildDate><image><url>https://garico92.github.io/website/media/sharing.png</url><title>Large-Scale Structure of the Universe; Cosmic Shear; Emulators;</title><link>https://garico92.github.io/website/tags/large-scale-structure-of-the-universe-cosmic-shear-emulators/</link></image><item><title>DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons</title><link>https://garico92.github.io/website/publications/desy3_analysis/</link><pubDate>Mon, 07 Aug 2023 00:00:00 +0000</pubDate><guid>https://garico92.github.io/website/publications/desy3_analysis/</guid><description>&lt;p&gt;This analyis was enabled by my previous work on a neural networks emulator trained on baryonified N-body simulations, described
.&lt;/p&gt;</description></item></channel></rss>