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EDP Sciences, EAS Publications Series, (40), p. 391-398

DOI: 10.1051/eas/1040054

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Cosmic microwave background science from Dome C

Journal article published in 2009 by P. de Bernardis ORCID, D. Barbosa ORCID, Y. Giraud-Héraud, M. Gervasi, E. Kreysa, B. Maffei, S. Masi ORCID, Philip Daniel Mauskopf, F. Pajot, L. Verde
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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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.