Estimating the spectral indices of correlated astrophysical foregrounds by a second-order statistical approach
We present the first tests of a new method, the correlated component analysis (CCA) based on second-order statistics, to estimate the mixing matrix, a key ingredient to separate astrophysical foregrounds superimposed to the Cosmic Microwave Background (CMB). In the present application, the mixing ma...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2006-11, Vol.373 (1), p.271-279 |
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Sprache: | eng |
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