Hervé Dole (IAS, Université Paris-Sud), Planck and the large scale structures
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Europe/Paris
LPNHE
LPNHE
Description
Planck, the European Space Agency's science cornerstone mission launched
in 2009 dedicated to cosmology, has measured the relic radiation from
the Big Bang (the Cosmic Microwave Background, CMB) with improved
sensitivity and resolution, in order to test theories on the birth and
evolution of the Universe and its large-scale content. In spring 2013,
we released the first cosmological results, and in early 2015 we will
release the final data. I will review the main results. In particular,
thanks to the best ever measured map of the CMB, we can improve our
knowledge about the age, content and evolution of our Universe, as well
as, for the first time, the very first moments (inflation) or the growth
of structures. Polarization results are also promissing. I will also
mention the technological challenge (the HFI instrument is cooled at
0.1K in space) that made this mission a success.
I will then focus on topics related to large scale structure, especially
galaxy clusters, cosmic infrared background with an emphasis of the
newly discovery of z>2 galaxies, lensed or clustered, confirmed by
Herschel.
More information:
- L'instrument HFI de Planck a été réalisé sous la maitrise
d'oeuvre de l'IAS et sous la responsabilité de Jean-Loup Puget
- Planck ESA web site:
http://www.esa.int/Our_Activities/Space_Science/Planck
- Planck papers: http://www.cosmos.esa.int/web/planck/publications