The Universe Traced by Clusters

dc.creatorSuto, Yasushi
dc.date2000-10-30
dc.date.accessioned2026-07-07T01:56:18Z
dc.date.available2026-07-07T01:56:18Z
dc.descriptionI critically review a methodology of using clusters of galaxies as cosmological probes. The understanding of the abundances and spatial correlations of dark matter halos has been significantly advanced especially for a last few years. Nevertheless such dark matter halos are not necessarily identical to clusters of galaxies in the universe. This is a quite obvious fact, but it seems that the resulting systematic errors, on the cosmological parameter estimates for instance, are often neglected in the literature.
dc.description10 pages, 8 figures. Invited talk at "Constructing the Universe with Clusters of Galaxies", IAP 2000 meeting, Paris (France) July 2000. To be published in the proceedings edited by Florence Durret & Daniel Gerbal
dc.identifierhttps://arxiv.org/abs/astro-ph/0010622
dc.identifierhttp://arxiv.org/abs/astro-ph/0010622
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1947
dc.subjectAstrophysics
dc.titleThe Universe Traced by Clusters
dc.typetext

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