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 fNL. We apply a third-order estimator of the needlet coefficients skewness and compute the χ2 statistics of its distribution. We obtain -80 < fNL < 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 fNL 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 fNL improve to -50 < fNL < 110 at 95 per cent confidence level.
Pietrobon, D., Cabella, P., Balbi, A., DE GASPERIS, G., Vittorio, N. (2009). Constraints on primordial non-Gaussianity from a needlet analysis of the WMAP-5 data. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 396, 1682-1688 [10.1111/j.1365-2966.2009.14847.x].
Constraints on primordial non-Gaussianity from a needlet analysis of the WMAP-5 data
CABELLA, PAOLO;BALBI, AMEDEO;DE GASPERIS, GIANCARLO;VITTORIO, NICOLA
2009-01-01
Abstract
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 fNL. We apply a third-order estimator of the needlet coefficients skewness and compute the χ2 statistics of its distribution. We obtain -80 < fNL < 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 fNL 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 fNL improve to -50 < fNL < 110 at 95 per cent confidence level.File | Dimensione | Formato | |
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