Bayesian joint estimation of non-Gaussianity and the power spectrum

Abstract

We propose a rigorous, non-perturbative, Bayesian framework which enables one jointly to test Gaussianity and estimate the power spectrum of CMB anisotropies. It makes use of the Hilbert space of an harmonic oscillator to set up an exact likelihood function, dependent on the power spectrum and on a set of parameters ${\alpha }_i$, which are zero for Gaussian processes. The latter can be expressed as series of cumulants; indeed they perturbatively reduce to cumulants. However they have the advantage that their variation is essentially unconstrained. Any truncation(i.e.: finite set of ${\alpha }_i$) therefore still produces a proper distribution - something which cannot be said of the only other such tool on offer, the Edgeworth expansion. We apply our method to Very Small Array (VSA) simulations based on signal Gaussianity, showing that our algorithm is indeed not biased.

11pages, 4 figures, submitted to MNRAS

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• Local non-Gaussianity in the Cosmic Microwave Background the Bayesian way
• Estimating the bispectrum of the Very Small Array data
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• Gaussianity of the CMB: Smooth Goodness of Fit Tests Applied to Interferometric Data
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• Markov Chain Beam Randomization: a study of the impact of PLANCK beam measurement errors on cosmological parameter estimation
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