4.7 Article

Constraints on primordial non-Gaussianity from a needlet analysis of the WMAP-5 data

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 396, Issue 3, Pages 1682-1688

Publisher

OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2009.14847.x

Keywords

methods: data analysis; cosmic microwave background; early Universe

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We look for a non-Gaussian signal in the Wilkinson Microwave Anisotropy Probe (WMAP) 5-year temperature anisotropy maps by performing a needlet-based data analysis. We use the foreground-reduced maps obtained by the WMAP team through the optimal combination of the W, V and Q channels, and perform realistic non-Gaussian simulations in order to constrain the non-linear coupling parameter f(NL). We apply a third-order estimator of the needlet coefficients skewness and compute the chi(2) statistics of its distribution. We obtain -80 < f(NL) < 120 at 95 per cent confidence level, which is consistent with a Gaussian distribution and comparable to previous constraints on the non-linear coupling. We then develop an estimator of f(NL) based on the same simulations and we find consistent constraints on primordial non-Gaussianity. We finally compute the three-point correlation function in needlet space: the constraints on f(NL) improve to -50 < f(NL) < 110 at 95 per cent confidence level.

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