Cosmic microwave background science from Dome C

de Bernardis, P., Barbosa, D., Giraud-Héraud, Y., Gervasi, M., Kreysa, E., Maffei, B., Masi, S., Mauskopf, Philip Daniel ORCID: https://orcid.org/0000-0001-6397-5516, Pajot, F. and Verde, L. 2010. Cosmic microwave background science from Dome C. Presented at: 3rd ARENA Conference, Frascati, Italy, 11-15 May 2009. Published in: Spinoglio, L. and Epchtein, N. eds. Proceedings of 3rd ARENA Conference on "An Astronomical Observatory at CONCORDIA (Dome C, Antarctica)", Frascati, Italy, 11-15 May 2009. EAS Publications Series. EAS Publication Series (40) Les Ulis, France: EDP Sciences, pp. 391-398. 10.1051/eas/1040054

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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.

Item Type:	Conference or Workshop Item (Paper)
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	EDP Sciences
ISBN:	9782759804856
ISSN:	16334760
Last Modified:	19 Oct 2022 10:40
URI:	https://orca.cardiff.ac.uk/id/eprint/25160

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