A Bayesian estimate of the skewness of the Cosmic Microwave Background

A Bayesian estimate of the skewness of the Cosmic Microwave Background

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We propose a formalism for estimating the skewness and angular power spectrum of a general Cosmic Microwave Background data set. We use the Edgeworth Expansion to define a non-Gaussian likelihood function that takes into account the anisotropic nature of the noise and the incompleteness of the sky c...

Полное описание

Библиографические подробности
Главные авторы:	Contaldi, C, Ferreira, P, Magueijo, J, Gorski, K
Формат:	Journal article
Опубликовано:	1999

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