The High-ell Excess In The CBI CMB Power Spectrum

Details The High-ell Excess In The CBI CMB Power Spectrum The High-ell Excess In The CBI CMB Power Spectrum

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...208.2704s&link_type=abstract

American Astronomical Society Meeting 208, #27.04; Bulletin of the American Astronomical Society, Vol. 38, p.106

Astronomy and Astrophysics

Astronomy

Scientific paper

Unexpectedly high power is observed in the Cosmic Microwave Background power spectrum on small angular scales (ell> 2000). Complementary optical and radio measurements should help constrain the source of the excess. We discuss the current state and follow-up observations of the high-ell excess, focusing in particular on data from the Cosmic Background Imager and follow-up data taken with the Canada-France-Hawaii telescope and the Green Bank Telescope.

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