Non-Gaussian Spectra in the Cosmic Microwave Background

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dc.creatorFerreira, Pedro G.
dc.date1997-02-19
dc.date.accessioned2026-07-07T02:22:57Z
dc.date.available2026-07-07T02:22:57Z
dc.descriptionWe 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)
dc.description3 pages, uses sprocl.sty
dc.identifierhttps://arxiv.org/abs/astro-ph/9702164
dc.identifierhttp://arxiv.org/abs/astro-ph/9702164
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11067
dc.subjectAstrophysics
dc.titleNon-Gaussian Spectra in the Cosmic Microwave Background
dc.typetext

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