Reconstructing cosmological density and velocity fields
I present a new quasi-linear method for reconstructing cosmological density and velocity fields from all-sky redshift surveys. The method is used to reconstruct the velocity field, dipole, bulk flows and distortion parameter <i>b</i> = Ω<sup>0.6</sup>/<i>b </i>fro...
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University of Edinburgh
2001
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.663167 |