<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Wasserman L. | Alex L Rojas</title><link>https://alexrojas.netlify.app/author/wasserman-l./</link><atom:link href="https://alexrojas.netlify.app/author/wasserman-l./index.xml" rel="self" type="application/rss+xml"/><description>Wasserman L.</description><generator>Source Themes Academic (https://sourcethemes.com/academic/)</generator><language>en-us</language><copyright>© 2025 Alex L Rojas</copyright><image><url>https://alexrojas.netlify.app/images/icon_hub400310ec8e000bf900e864bd27caf38_19701_512x512_fill_lanczos_center_2.png</url><title>Wasserman L.</title><link>https://alexrojas.netlify.app/author/wasserman-l./</link></image><item><title>Revealing components of the galaxy population through non-parametric techniques</title><link>https://alexrojas.netlify.app/publication/2008-12-01_nmr/</link><pubDate>Mon, 01 Dec 2008 00:00:00 +0000</pubDate><guid>https://alexrojas.netlify.app/publication/2008-12-01_nmr/</guid><description/></item></channel></rss>