<rdf:RDF xmlns:rdf="http://www.openarchives.org/OAI/2.0/rdf/" xmlns:ow="http://www.ontoweb.org/ontology/1#" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:ds="http://dspace.org/ds/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/rdf/ http://www.openarchives.org/OAI/2.0/rdf.xsd">
   <ow:Publication rdf:about="oai:digibug.ugr.es:10481/48888">
      <dc:title>A multy-frequency study of the SFHS of galaxies in the integral field area survey CALIFA</dc:title>
      <dc:creator>López Fernández, Rafael</dc:creator>
      <dc:contributor>González Delgado, Rosa María</dc:contributor>
      <dc:contributor>Cid Fernandes, Roberto</dc:contributor>
      <dc:contributor>Universidad de Granada. Programa Oficial de Doctorado en Física y Matemáticas</dc:contributor>
      <dc:contributor>Consejo Superior de Investigaciones Científicas (CSIC). Instituto de Astrofísica de Andalucía</dc:contributor>
      <dc:subject>Galaxias</dc:subject>
      <dc:subject>Evolución</dc:subject>
      <dc:subject>Dinámica galáctica</dc:subject>
      <dc:subject>Espectroscopía astronómica</dc:subject>
      <dc:subject>Materia interestelar</dc:subject>
      <dc:subject>Astrofísica</dc:subject>
      <dc:subject>Fotometría astronómica</dc:subject>
      <dc:description>The study in this thesis is based on the statistical analysis of the stellar population properties of&#xd;
galaxies, combining di↵erent kinds of data. In particular we use Integral Field Spectroscopy (IFS)&#xd;
provided by CALIFA data and images in optical and UV range provided by SDSS and GALEX,&#xd;
respectively. The main goal is to obtain the cosmic evolution of the star formation and mass assembly&#xd;
history of galaxies using integrated and spatially resolved information of galaxies in the near Universe.&#xd;
The objects in this study are those for which CALIFA+GALEX+SDSS data are available. This is&#xd;
a sub-sample of 366 galaxies which is unbiased with respect to the CALIFA mother sample, including&#xd;
from E to late type spirals and with M? from 109 to 8⇥1011 M!. The CALIFA mother sample is not a&#xd;
purely volume-limited sample, but can be “volume-corrected”. As the sub-sample is representative of&#xd;
the CALIFA mother sample, our results can be used to estimate the star formation rate density (⇢SFR),&#xd;
the specific SFR (sSFR) and the stellar mass density (⇢Mass) up to z > 2, and the contribution of&#xd;
central (&lt;0.5 HLR) and outermost regions (1 &lt; R &lt; 2 HLR) in nearby galaxies to these fundamental&#xd;
observables in astrophysical cosmology.</dc:description>
      <dc:date>2018-01-15T10:18:35Z</dc:date>
      <dc:date>2018-01-15T10:18:35Z</dc:date>
      <dc:date>2017</dc:date>
      <dc:date>2017-09-29</dc:date>
      <dc:type>doctoral thesis</dc:type>
      <dc:identifier>López Fernández, R. A multy-frequency study of the SFHS of galaxies in the integral field area survey CALIFA. Granada: Universidad de Granada, 2017. [http://hdl.handle.net/10481/48888]</dc:identifier>
      <dc:identifier>9788491636922</dc:identifier>
      <dc:identifier>http://hdl.handle.net/10481/48888</dc:identifier>
      <dc:language>eng</dc:language>
      <dc:language>spa</dc:language>
      <dc:rights>http://creativecommons.org/licenses/by-nc-nd/3.0/</dc:rights>
      <dc:rights>open access</dc:rights>
      <dc:rights>Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License</dc:rights>
      <dc:publisher>Universidad de Granada</dc:publisher>
   </ow:Publication>
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