Cosmic Microwave Fluctuations, Present and Future

Details Cosmic Microwave Fluctuations, Present and Future Cosmic Microwave Fluctuations, Present and Future

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cpa..conf...14b&link_type=abstract

PROCEEDINGS OF THE 2002 INTERNATIONAL SYMPOSIUM ON COSMOLOGY AND PARTICLE ASTROPHYSICS (CosPA 02). Held 31 May ?2 June 2002 in T

Astronomy and Astrophysics

Astrophysics

Scientific paper

The knowledge of the characteristics of the cosmic Microwave Background (CMB) anisotropies has been fast and steadily increasing over the last few years. After a brief historical overview, I show that a consistent picture has emerged, from the analysis of CMB data alone, from the analysis of Large Scale Structures (LSS) data, and from their combination. I then review the status of the ARCHEOPS balloon borne experiment whose first results should be available within the same time frame than those of MAP. I will then present what to expect from the two satellite projects in this area, the MAP experiment which is currently operating, and the Planck experiment which should be launched mid-2007.

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