Cosmic microwave background snapshots: pre-WMAP and post-WMAP

Author:

Bond J. Richard123,Contaldi Carlo1,Pogosyan Dmitry4

Affiliation:

1. Canadian Institute for Advanced Research, Cosmology and Gravity Program, Canadian Institute for Theoretical Astrophysics, McLennan Physical Laboratories, University of Toronto, 60 St George Street, Toronto, Ontario M5S 3H8, Canada

2. Institut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014 Paris, France

3. Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK

4. Department of Physics, University of Alberta, 412 Avadh Bhatia Physics Laboratory, Edmonton, Alberta T6G 2J1, Canada

Publisher

The Royal Society

Subject

General Physics and Astronomy,General Engineering,General Mathematics

Reference3 articles.

1. First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic Results

2. Benoit A. etal . 2002 Astron. Astrophys. 399 L19{L25.

3. Bond J. R. 1996 Cosmology and large scale structure. Les Houches Session LX (ed. R. Schae® er J. Silk M. Spiro & J. Zinn-Justin) pp. 469{674. Elsevier. (Available at http://

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