Astrophysical component separation of COBE-DMR 4-yr data with FastICA

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Astrophysical components separation of COBE-DMR 4yr data with FastICA

We present an application of the fast Independent Component Analysis FastICA method to the COBE-DMR 4yr data. Although the signal-to-noise ratio in the COBE-DMR data is typically ∼ 1, the approach is able to extract the CMB signal with high confidence when working at high galactic latitudes. However, the foreground emission components have too low a S/N ratio to be reconstructed by this method ...

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ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 2003

ISSN: 0035-8711,1365-2966

DOI: 10.1046/j.1365-8711.2003.06835.x