EAS Publications Series
Volume 40, 20103rd ARENA Conference: An Astronomical Observatory at CONCORDIA (Dome C, Antarctica)
|Page(s)||391 - 398|
|Published online||23 December 2009|
L. Spinoglio and N. Epchtein (eds)
EAS Publications Series, 40 (2010) 391-398
Cosmic Microwave Background science from Dome C
Dipartimento di Fisica, Universitá di Roma La Sapienza, Italy
2 Grupo de RadioAstronomia, Instituto de Telecomunicações, Aveiro, Portugal
3 APC Paris, France
4 Dipartimento di Fisica, Universitá di Milano Bicocca, Italy
5 Max Planck Radioastronomie, Bonn, Germany
6 University of Manchester, UK
7 Department of Physics and Astronomy, University of Cardiff, UK
8 IAS Orsay, France
9 Institute of Space Sciences, Bellaterra, Spain
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.
© EAS, EDP Sciences, 2010
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.