Cosmic microwave background science from Dome C

P. De Bernardis; D. Barbosa; Y. Giraud-Héraud; M. Gervasi; E. Kreysa; B. Maffei; S. Masi; P. Mauskopf; F. Pajot; L. Verde

doi:10.1051/eas/1040054

Cosmic microwave background science from Dome C

P. De Bernardis, D. Barbosa, Y. Giraud-Héraud, M. Gervasi, E. Kreysa, B. Maffei, S. Masi, P. Mauskopf, F. Pajot, L. Verde

Research output: Contribution to journal › Article › peer-review

2 Scopus citations

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.

Original language	English (US)
Pages (from-to)	391-398
Number of pages	8
Journal	EAS Publications Series
Volume	40
DOIs	https://doi.org/10.1051/eas/1040054
State	Published - 2010
Externally published	Yes

ASJC Scopus subject areas

Astronomy and Astrophysics
General Engineering
Space and Planetary Science

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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.",

author = "{De Bernardis}, P. and D. Barbosa and Y. Giraud-H{\'e}raud and M. Gervasi and E. Kreysa and B. Maffei and S. Masi and P. Mauskopf and F. Pajot and L. Verde",

year = "2010",

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AU - De Bernardis, P.

AU - Barbosa, D.

AU - Giraud-Héraud, Y.

AU - Gervasi, M.

AU - Kreysa, E.

AU - Maffei, B.

AU - Masi, S.

AU - Mauskopf, P.

AU - Pajot, F.

AU - Verde, L.

PY - 2010

Y1 - 2010

N2 - 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.

AB - 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.

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DO - 10.1051/eas/1040054

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JO - EAS Publications Series

JF - EAS Publications Series

ER -

Cosmic microwave background science from Dome C

Abstract

ASJC Scopus subject areas

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