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Cosmological Non-Gaussian Signature Detection: Comparing Performance of Different Statistical Tests
<p/> <p>Currently, it appears that the best method for non-Gaussianity detection in the cosmic microwave background (CMB) consists in calculating the kurtosis of the wavelet coefficients. We know that wavelet-kurtosis outperforms other methods such as the bispectrum, the genus, ridgelet-...
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Main Authors: | , , , , |
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Formato: | Artigo |
Idioma: | Inglês |
Publicado em: |
SpringerOpen
2005-01-01
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Colecção: | EURASIP Journal on Advances in Signal Processing |
Assuntos: | |
Acesso em linha: | http://dx.doi.org/10.1155/ASP.2005.2470 |
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