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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