Panel Review: Reconstruction Methods and the Value of $β$

dc.creatorWillick, Jeffrey A.
dc.date1999-09-01
dc.date.accessioned2026-07-07T02:32:59Z
dc.date.available2026-07-07T02:32:59Z
dc.descriptionThe closely related issues of (1) reconstructing density and velocity fields from redshift survey and distance indicator data and (2) determining cosmological parameters from such data sets are discussed. I focus on possible explanations for the discrepant values of $β\equivΩ^{0.6}/b$ resulting from analyses that employ various reconstruction methods. Although no firm conclusions are reached, possible routes towards resolution of these discrepancies are suggested by the discussion.
dc.description4 pages, 1 figure, Cosmic Flows Workshop, Victoria BC, July 1999, S. Courteau, M. Strauss, and J. Willick eds
dc.identifierhttps://arxiv.org/abs/astro-ph/9909003
dc.identifierhttp://arxiv.org/abs/astro-ph/9909003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14669
dc.subjectAstrophysics
dc.titlePanel Review: Reconstruction Methods and the Value of $β$
dc.typetext

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