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The Jodrell Bank - IAC 33 GHz Interferometer

  • D. L. Harrison (a1), R. A. Watson (a1), J. A. Rubiño-Martin (a2), J. F. Macias-Perez (a1), R. D. Davies (a1), R. Rebolo (a2), C. M. Gutiérrez (a2) and R. J. Davis (a1)...


This paper presents results obtained with the Jodrell Bank - IAC two-element 33 GHz interferometer, located at the Teide Observatory on Tenerife, which is designed to measure the level of the Cosmic Microwave Background (CMB) fluctuations on angular scales of 1° and 2°. The result from a maximum likelihood analysis of observations taken at Dec +41° of δT l = 63+7 -6μK at l = 208 ± 18 is comparable with those of Boomerang and Maxima. The contribution of possible foreground contaminants are considered.



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