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 <identifier>oai:arXiv.org:1604.05585</identifier>
 <datestamp>2016-04-20</datestamp>
 <setSpec>physics:astro-ph</setSpec>
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 <id>1604.05585</id><created>2016-04-19</created>
<authors>
<author><keyname>Burigana</keyname><forenames>Günter</forenames><affiliation>on behalf of Planck Collaboration</affiliation></author>
<author><keyname>Trombetti</keyname><forenames>Tiziana</forenames><affiliation>on behalf of Planck Collaboration</affiliation></author>
<author><keyname>Paoletti</keyname><forenames>Daniela</forenames><affiliation>on behalf of Planck Collaboration</affiliation></author>
<author><keyname>Mandolesi</keyname><forenames>Nazzareno</forenames><affiliation>on behalf of Planck Collaboration</affiliation>
</author><author><keyname>Natoli</keyname><forenames>Paolo</forenames><affiliation>on behalf of Planck Collaboration</affiliation></author>
</authors>
<title>Astrophysical components from Planck maps</title><categories>astro-ph.GA astro-ph.CO</categories><comments>4 pages, 2 figures. It will appear on the Proceedings of the 17th
  Lomonosov Conference on Elementary Particle Physics. Moscow State University,
  Moscow, 20-26 August, 2015. Invited talk</comments><license>http://arxiv.org/licenses/nonexclusive-distrib/1.0/</license><abstract>  The Planck Collaboration has recently released maps of the microwave sky in
both temperature and polarization. Diffuse astrophysical components (including
Galactic emissions, cosmic far infrared (IR) background, y-maps of the thermal
Sunyaev-Zeldovich (SZ) effect) and catalogs of many thousands of Galactic and
extragalactic radio and far-IR sources, and galaxy clusters detected through
the SZ effect are the main astrophysical products of the mission. A concise
overview of these results and of astrophysical studies based on Planck data is
presented.
</abstract></arXiv>
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