<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>TRICEPS | Borja Perez-Diaz</title><link>https://borja-perez-diaz.github.io/me/tags/triceps/</link><atom:link href="https://borja-perez-diaz.github.io/me/tags/triceps/index.xml" rel="self" type="application/rss+xml"/><description>TRICEPS</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Tue, 01 Jul 2025 00:00:00 +0000</lastBuildDate><image><url>https://borja-perez-diaz.github.io/me/media/icon_hu7729264130191091259.png</url><title>TRICEPS</title><link>https://borja-perez-diaz.github.io/me/tags/triceps/</link></image><item><title>TRICEPS - Tracing Rotation with Ionized Carbon in Early Primeval Systems</title><link>https://borja-perez-diaz.github.io/me/project/triceps/</link><pubDate>Tue, 01 Jul 2025 00:00:00 +0000</pubDate><guid>https://borja-perez-diaz.github.io/me/project/triceps/</guid><description>&lt;p>TRICEPS is a survey of 15 massive galaxies at z=4-5, when the Universe was less than 1.5 Gyr old. TRICEPS combines new observations from ALMA, JWST, and the VLA, as well as ancillary data from HST, Spitzer, and Herschell.&lt;/p>
&lt;p>The main goal is of TRICEPS is to trace the distribution of baryons and dark matter in the most distant rotation-supported galaxies, using ALMA [CII] data to trace the rotation curve, JWST NIR data to trace the stellar mass, and VLA CO(1-0) data to trace the gas mass.&lt;/p>
&lt;p>The P.I: of the project is Prof. Federico Lelli.&lt;/p></description></item></channel></rss>