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. © 2010 EAS, EDP Sciences.

de Bernardis, P., Barbosa, D., Giraud Heraud, Y., Gervasi, M., Kreysa, E., Maffei, B., et al. (2010). Cosmic Microwave Background science from Dome C. In 3rd ARENA Conference: An Astronomical Observatory at CONCORDIA (Dome C, Antarctica) (pp.391-398) [10.1051/eas/1040054].

Cosmic Microwave Background science from Dome C

GERVASI, MASSIMO;
2010

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. © 2010 EAS, EDP Sciences.
paper
Cosmology, Cosmic microwave background
English
3rd ARENA Conference: An Astronomical Observatory at CONCORDIA (Dome C, Antarctica)
2009
3rd ARENA Conference: An Astronomical Observatory at CONCORDIA (Dome C, Antarctica)
2010
40
391
398
none
de Bernardis, P., Barbosa, D., Giraud Heraud, Y., Gervasi, M., Kreysa, E., Maffei, B., et al. (2010). Cosmic Microwave Background science from Dome C. In 3rd ARENA Conference: An Astronomical Observatory at CONCORDIA (Dome C, Antarctica) (pp.391-398) [10.1051/eas/1040054].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/21816
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