Redshift Distortions and Clustering in the PSCz Survey

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dc.creatorBallinger, W. E.
dc.creatorTaylor, A. N.
dc.creatorHeavens, A. F.
dc.creatorTadros, H.
dc.date2000-05-04
dc.date.accessioned2026-07-07T01:53:22Z
dc.date.available2026-07-07T01:53:22Z
dc.descriptionWe have constrained the redshift-distortion parameter $β\equiv Ω^{0.6}/b$ 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, $β=0.4 \pm 0.1$, strongly rules out $β=1$.
dc.description4 pages, 2 figures, contribution to the Proceedings of Moriond 2000 "Energy Densities in the Universe", Les Arcs, France, January 22-29 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0005094
dc.identifierhttp://arxiv.org/abs/astro-ph/0005094
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/949
dc.subjectAstrophysics
dc.titleRedshift Distortions and Clustering in the PSCz Survey
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