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Cosmic Microwave Background science from Dome C

Published online by Cambridge University Press:  24 December 2009

L. Spinoglio ,
N. Epchtein ,
P. de Bernardis ,
D. Barbosa ,
Y. Giraud-Héraud ,
M. Gervasi ,
E. Kreysa ,
B. Maffei ,
S. Masi  and
P. Mauskopf
...Show all authors
P. de Bernardis
Affiliation:
Dipartimento di Fisica, Universitá di Roma La Sapienza, Italy
D. Barbosa
Affiliation:
Grupo de RadioAstronomia, Instituto de Telecomunicações, Aveiro, Portugal
Y. Giraud-Héraud
Affiliation:
APC Paris, France
M. Gervasi
Affiliation:
Dipartimento di Fisica, Universitá di Milano Bicocca, Italy
E. Kreysa
Affiliation:
Max Planck Radioastronomie, Bonn, Germany
B. Maffei
Affiliation:
University of Manchester, UK
S. Masi
Affiliation:
Dipartimento di Fisica, Universitá di Roma La Sapienza, Italy
P. Mauskopf
Affiliation:
Department of Physics and Astronomy, University of Cardiff, UK
F. Pajot
Affiliation:
IAS Orsay, France
L. Verde
Affiliation:
Institute of Space Sciences, Bellaterra, Spain
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Abstract

We summarize the results of the Cosmic Microwave Background (CMB) working group of the ARENA project. The focus has been on precision measurements of CMB polarization (looking for the echoes of cosmological inflation) and high angular resolution CMB measurements (looking for Sunyaev Zeldovich effect in distant clusters of Galaxies, to probe the evolution of the Universe, Dark Matter and Dark Energy). For both projects the Dome C site represents the best choice worldwide.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 40: 3rd ARENA Conference: An Astronomical Observatory at CONCORDIA (Dome C, Antarctica) , 2010 , pp. 391 - 398
Copyright
© EAS, EDP Sciences, 2010

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