A Measurement of the Angular Power Spectrum of the Microwave Background Made from the High Chilean Andes

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Published 1999 July 28 © 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation E. Torbet et al 1999 ApJ 521 L79 DOI 10.1086/312197

1538-4357/521/2/L79

Abstract

We report on a measurement of the angular spectrum of the anisotropy of the microwave sky at 30 and 40 GHz between l = 50 and l = 200. The data, covering roughly 600 deg2, support a rise in the angular spectrum to a maximum with δTl ≈ 85 μK at l = 200. We also give a 2 σ upper limit of δTl < 122 μK at l = 432 at 144 GHz. These results come from the first campaign of the Mobile Anisotropy Telescope on Cerro Toco, Chile. To assist in assessing the site, we present plots of the fluctuations in atmospheric emission at 30 and 144 GHz.

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10.1086/312197