Non-Gaussian Spectra in the Cosmic Microwave Background
Pedro G. Ferreira
Abstract
We propose a set of new statistics which can be extracted out of the angular distribution of the Fourier transform of the temperature anisotropies in the small field limit. They quantify generic non-Gaussian structure and complement the power spectrum in characterizing the sampled distribution function of a data set (contribution to the 18th Texas Symposium Proceedings)
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