%0 Journal Article
%T Redshift Distortions and Clustering in the PSCz Survey
%A W. E. Ballinger
%A A. N. Taylor
%A A. F. Heavens
%A H. Tadros
%J Physics
%D 2000
%I arXiv
%X We have constrained the redshift-distortion parameter $\beta \equiv \Omega^{0.6}/b$ and the real-space power spectrum of the IRAS PSCz survey using a spherical-harmonic redshift-distortion analysis combined with a data compression method which is designed to deal with correlated parameters. Our latest result, $\beta=0.4 \pm 0.1$, strongly rules out $\beta=1$.
%U http://arxiv.org/abs/astro-ph/0005094v1