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Aug 2, 2002 · This paper is the fourth in a series devoted to the inverse scattering problem (ISP) which arises in the context of tomographic imaging with ...
Non-linear evolution causes the galaxy power spectrum to become broadly correlated over different wavenumbers. It is shown that pre-whitening the power ...
We shall give a proof of (2.1.1) by the centroid method in Section 3. 2.2. CebySev's inequality. Let a = (aļ9 . . . , an) ...
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