A Measurement of the Angular Power Spectrum of the CMB from l = 100 to 400
arXiv:astro-ph/9906421 · doi:10.1086/312293
Abstract
We report on a measurement of the angular spectrum of the CMB between and made at 144 GHz from Cerro Toco in the Chilean altiplano. When the new data are combined with previous data at 30 and 40 GHz, taken with the same instrument observing the same section of sky, we find: 1) a rise in the angular spectrum to a maximum with K at and a fall at , thereby localizing the peak near ; and 2) that the anisotropy at has the spectrum of the CMB.
4 pages, 2 figures. Revised version; includes Ned Wright's postscript fix. Accepted by ApJL. Website at http://physics.princeton.edu/~cmb/
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