<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>L. Hebb | Santiago Páez Avendaño</title><link>https://s-paez.github.io/author/l.-hebb/</link><atom:link href="https://s-paez.github.io/author/l.-hebb/index.xml" rel="self" type="application/rss+xml"/><description>L. Hebb</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Wed, 11 Mar 2026 00:00:00 +0000</lastBuildDate><image><url>https://s-paez.github.io/media/icon_hu9827122857082748793.png</url><title>L. Hebb</title><link>https://s-paez.github.io/author/l.-hebb/</link></image><item><title>Data reduction method for OPTICAM multiband time series of transiting exoplanets</title><link>https://s-paez.github.io/publication/profe_paper/</link><pubDate>Wed, 11 Mar 2026 00:00:00 +0000</pubDate><guid>https://s-paez.github.io/publication/profe_paper/</guid><description/></item></channel></rss>