AAS 199th meeting, Washington, DC, January 2002
Session 34. Cosmic Microwave Background Anisotropy and Dark Matter
Oral, Monday, January 7, 2002, 2:00-3:30pm, International Ballroom East

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[34.02] The CMB Power Spectrum from CBI Mosaics

J.L. Sievers, T.J. Pearson, A.C.S. Readhead, M.C. Shepherd, P.S. Udomprasert, J.K. Cartwright, B.S. Mason, S. Padin (Caltech), S.T. Myers (NRAO), J.R. Bond, C. Contaldi, S. Prunet, D. Pogosyan (CITA)

The Cosmic Background Imager is a thirteen element interferometer located in Chilean Andes designed to measure the angular power spectrum of the Cosmic Microwave Background. It uses low-noise HEMT receivers covering the frequency range of 26-36 GHz. We present the power spectrum to l=2000 measured by CBI from three 2x2 degree mosaics of 42 pointings each and discuss the implications of the results.

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The author(s) of this abstract have provided an email address for comments about the abstract: js@astro.caltech.edu

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