Component separation for Cosmic Microwave Background data: a blind approach based on spectral diversity
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[1] A. H. Jarrett,et al. A New Astronomy , 1898, Nature.
[2] Max Tegmark,et al. A method for subtracting foregrounds from multifrequency CMB sky maps , 1996 .
[3] C. Frenk,et al. The Evolution of X-Ray Clusters in a Low-Density Universe , 1997, astro-ph/9708070.
[4] A. Lasenby,et al. Foreground separation methods for satellite observations of the cosmic microwave background , 1998, astro-ph/9806387.
[5] E. Hivon,et al. Analysis issues for large CMB data sets , 1998, astro-ph/9812350.
[6] Matias Zaldarriaga,et al. CMBFAST for Spatially Closed Universes , 1999, astro-ph/9911219.
[7] C. Baccigalupi,et al. Neural networks and the separation of cosmic microwave background and astrophysical signals in sky maps , 2000, astro-ph/0002257.
[8] L. Toffolatti,et al. Combining maximum-entropy and the Mexican hat wavelet to reconstruct the microwave sky , 2001 .
[9] Error estimation for the MAP experiment , 2000, astro-ph/0012497.
[10] M. Hobson,et al. All-sky component separation for the Planck mission , 2001, astro-ph/0105432.
[11] Hichem Snoussi,et al. Blind separation of noisy Gaussian stationary sources. Application to cosmic microwave background imaging , 2002, 2002 11th European Signal Processing Conference.
[12] G. Zotti,et al. All-sky astrophysical component separation with Fast Independent Component Analysis (FastICA) , 2001, astro-ph/0108362.
[13] J. Cardoso,et al. Multidetector multicomponent spectral matching and applications for cosmic microwave background data analysis , 2002, astro-ph/0211504.
[14] Richard Gispert,et al. Semi-analytical estimates of contamination , 2008 .