Non-Gaussian Spectra in the Cosmic Microwave Background
Abstract
Description
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)
3 pages, uses sprocl.sty
3 pages, uses sprocl.sty