English

A high-significance detection of non-Gaussianity in the WMAP 3-year data using directional spherical wavelets

Astrophysics 2011-02-11 v2

Abstract

We repeat the directional spherical real Morlet wavelet analysis used to detect non-Gaussianity in the WMAP 1-year data (McEwen et al. 2005a), on the WMAP 3-year data. The non-Gaussian signal previously detected is indeed present in the 3-year data, although the significance of the detection is reduced. Using our most conservative method for constructing significance measures, we find the significance of the detection of non-Gaussianity drops from 98.3+/-0.4% to 94.9+/-0.7%; the significance drops from 99.3+/-0.3% to 97.2+/-0.5% using a method based on the χ2\chi^2 statistic. The wavelet analysis allows us to localise most likely sources of non-Gaussianity on the sky. We detect very similar localised regions in the WMAP 1-year and 3-year data, although the regions extracted appear more pronounced in the 3-year data. When all localised regions are excluded from the analysis the 3-year data is consistent with Gaussianity.

Keywords

Cite

@article{arxiv.astro-ph/0604305,
  title  = {A high-significance detection of non-Gaussianity in the WMAP 3-year data using directional spherical wavelets},
  author = {J. D. McEwen and M. P. Hobson and A. N. Lasenby and D. J. Mortlock},
  journal= {arXiv preprint arXiv:astro-ph/0604305},
  year   = {2011}
}

Comments

5 pages, 5 figures; typographical changes to match version accepted by MNRAS