<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Authors | Linda Blot</title><link>https://46306e0b.my-hugo-academic-website.pages.dev/authors/</link><atom:link href="https://46306e0b.my-hugo-academic-website.pages.dev/authors/index.xml" rel="self" type="application/rss+xml"/><description>Authors</description><generator>Source Themes Academic (https://sourcethemes.com/academic/)</generator><language>en-us</language><copyright>© 2018</copyright><image><url>img/map[gravatar:%!s(bool=false) shape:circle]</url><title>Authors</title><link>https://46306e0b.my-hugo-academic-website.pages.dev/authors/</link></image><item><title/><link>https://46306e0b.my-hugo-academic-website.pages.dev/authors/admin/</link><pubDate>Mon, 01 Jan 0001 00:00:00 +0000</pubDate><guid>https://46306e0b.my-hugo-academic-website.pages.dev/authors/admin/</guid><description>&lt;p>My research work focuses on cosmological simulations in the context of data analysis for large galaxy surveys. In particular, I work on modelling galaxy clustering and weak lensing observables and their statistical properties using simulations.&lt;/p>
&lt;p>I am member of the
&lt;a href="https://www.euclid-ec.org" target="_blank" rel="noopener">Euclid Consortium&lt;/a>, for which I produced large galaxy mock catalogues for testing the performances of the Euclid satellite, in collaboration with the Spanish Euclid data center at
&lt;a href="https://www.pic.es" target="_blank" rel="noopener">PIC&lt;/a>.&lt;/p>
&lt;p>I am part of the
&lt;a href="http://www.edecs.org" target="_blank" rel="noopener">Exploring Dark Energy through Cosmic Structures&lt;/a> project, for which I develop numerical methods to perform cosmological simulations of clustering dark energy scenarios.&lt;/p></description></item></channel></rss>