Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...199.3402s&link_type=abstract
American Astronomical Society, 199th AAS Meeting, #34.02; Bulletin of the American Astronomical Society, Vol. 33, p.1357
Astronomy and Astrophysics
Astronomy
1
Scientific paper
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.
Bond Richard J.
Cartwright John K.
Contaldi Carlo
Mason Brian S.
Myers Steven T.
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