<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Projects | Borja Perez-Diaz</title><link>https://borja-perez-diaz.github.io/me/project/</link><atom:link href="https://borja-perez-diaz.github.io/me/project/index.xml" rel="self" type="application/rss+xml"/><description>Projects</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>Projects</title><link>https://borja-perez-diaz.github.io/me/project/</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><item><title>Estallidos</title><link>https://borja-perez-diaz.github.io/me/project/estallidos/</link><pubDate>Mon, 01 Feb 2021 00:00:00 +0000</pubDate><guid>https://borja-perez-diaz.github.io/me/project/estallidos/</guid><description>&lt;p>ESTALLIDOS is a coordinated project between several Spanish research centers to study the formation and evolution of outbursts of star formation.&lt;/p>
&lt;p>The project is aimed at studying massive starbursts and their impact on galaxies, using both observational and theoretical tools. We observe starbursts and model the physical processes that are involved, paying particular attention to the feedback on the surroundings that quenches or stimulates the formation of successive generations of stars.&lt;/p>
&lt;p>The project began in December 2001, in a collaboration among astronomers from the LAEFF (Madrid; currently integrated into the CAB ), the VILSPA (Madrid, currently ESAC ), the IAA (Granada), and the IAC (Canary Islands) funded by the Spanish Plan Nacional de Astronomía y Astrofísica ( AYA2001-3939-C03 ). From the beginning, the project has involved the participation of researchers from all over the world. In later editions, UAM , and, posteriorly CIEMAT (Madrid) joined the project. Details about the different funded projects can be found in the Organization Chart and Operations item in the left menu.&lt;/p>
&lt;p>Now we are in the eighth edition: ESTALLIDOS 8 : Las diversas facetas de la formación estelar en el Universo (PID2022-136598NB-C31, C32 and C33) which is coordinated by the IAC node.&lt;/p>
&lt;p>The project is organized and coordinated through workshops in which ongoing work is discussed and new results are presented. They are attended by a significant part of the Estallidos community ( currently around 60 ) and help to maintain strong scientific bounds and close collaborations.&lt;/p></description></item></channel></rss>