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<p>Buenos dias a tod@s,<br>
<br>
Espero se encuentren muy bien.<br>
<br>
Por este medio, quisiera enviarles un <b>último recordatorio</b> acerca del curso sobre ajuste de distribucion espectral de energia (SED fitting), a cargo del Dr. Roberto Cid Fernandes, de la Universidad de Santa Catarina (Brasil), que nos encontramos organizando desde el grupo de investigación <a data-saferedirecturl="https://www.google.com/url?q=https://sites.google.com/view/alas-ialp-fcaglp/activities/courses?authuser%3D0&source=gmail&ust=1727453579698000&usg=AOvVaw3jE0qu6CMSssSx0CIZzguu" href="https://sites.google.com/view/alas-ialp-fcaglp/activities/courses?authuser=0" style="color: rgb(17, 85, 204);" target="_blank">"Astrophysics with Large Astronomical Surveys" (ALAS)</a>. A los fines de ultimar detalles y organizar un doodle para decidir los mejores horarios para l@s participantes, agradeceriamos a quienes se encuentren interesados en asistir, <b>y que aun no lo hayan hecho</b>, me envien <b>antes del próximo Martes 1 de Octubre </b>un mensaje a <a href="mailto:asmith@fcaglp.unlp.edu.ar" style="color: rgb(17, 85, 204);" target="_blank">asmith@fcaglp.unlp.edu.ar</a> manifestando su interes. Luego de esa fecha, los mails relacionados con el curso solo seran enviados a la lista de interesad@s.<br>
<br>
Al pie les dejo la informacion con la que contamos hasta el momento sobre el mencionado curso. Cualquier consulta, no duden en escribirme.<br>
<br>
Abrazo.<br>
<br>
Analía.<br>
<br>
==============================<wbr>========<br>
<br></p>
<div style="text-align: center;"><b>Spectral Synthesis of Stellar Populations in Galaxies</b></div>
<div style="text-align: center;"><b>14-18 October 2024 - FCAG</b></div>
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Galaxy spectra and/or multi-band photometry are the major source of<br>
knowledge about galaxy evolution through cosmic times. The translation of observed fluxes to physical properties like stellar masses, mean stellar, metallicities, and the star formation history involves several astrophysical ingredients and mathematical/methodological issues. Basic knowledge of these topics is necessary for a minimal understanding of a large part of the current (and past) literature on extragalactic astronomy. These series of lectures cover these topics. The aim is not to present the latest, more sophisticated spectral synthesis tools in the field, but, instead, to ensure the students have a basic understanding of the ingredients, assumptions, and limitations of such tools. The course will consist of <b>four lectures of 2 hours, plus four ~ 1 hour lectures for practical (jupyter notebook-based) work.</b><br></p>
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<div dir="ltr" style="color: rgb(32, 33, 36); font-family: Arial, Helvetica, sans-serif; font-size: small; background-color: rgb(255, 255, 255);"><font color="#000000"><font face="arial, sans-serif">Geof. Mercedes Gil </font><br>
<font face="arial, sans-serif">Secretaria de Posgrado </font></font></div>
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<div dir="ltr" style="color: rgb(32, 33, 36); font-family: Arial, Helvetica, sans-serif; font-size: small; background-color: rgb(255, 255, 255);"><font color="#000000" face="arial, sans-serif">Facultad de Ciencias Astronómicas y Geofísicas<br>
Universidad Nacional de La Plata</font>
<div><font color="#000000" face="arial, sans-serif"><b style="line-height: 16.5px; background-color: rgb(252, 252, 252);">Teléfono</b><span style="line-height: 16.5px; background-color: rgb(252, 252, 252);">: (0221) - 423 - 6593 int. 1050</span><br>
<a href="http://www.fcaglp.unlp.edu.ar/area-docente/posgrado/posgrado" style="margin: 0px; padding: 0px; outline: none; background-image: initial; background-position: initial; background-repeat: initial;" target="_blank">http://www.fcaglp.unlp.edu.ar/posgrados</a></font><br>
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