Open AccessThe performance of spherical wavelets to detect non‐Gaussianity in the cosmic microwave background sky
Author(s) -
MartínezGonzález E.,
Gallegos J. E.,
Argüeso F.,
Cayón L.,
Sanz J. L.
Publication year - 2002
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2002.05648.x
Subject(s) - kurtosis , wavelet , physics , cosmic microwave background , skewness , gaussian , non gaussianity , statistical physics , astron , bispectrum , cosmic background radiation , astrophysics , statistics , optics , artificial intelligence , spectral density , mathematics , quantum mechanics , computer science , anisotropy
We investigate the performance of spherical wavelets in discriminating between standard inflationary (Gaussian) and non‐Gaussian models. For the latter we consider small perturbations of the Gaussian model in which an artificially specified skewness or kurtosis is introduced through the Edgeworth expansion. By combining all the information present in all the wavelet scales with the Fisher discriminant, we find that the spherical Mexican Hat wavelets are clearly superior to the spherical Haar wavelets. The former can detect levels of skewness and kurtosis of ≈1 per cent for 33‐arcmin resolution, an order of magnitude smaller than the latter. Also, as expected, both wavelets are better for discriminating between the models than the direct consideration of moments of the temperature maps. The introduction of instrumental white noise in the maps, S / N = 1 , does not change the main results of this paper.