3D Identification and Reconstruction of z~1 Clusters: Prospects for the DEEP2 Redshift Survey

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dc.creatorMarinoni, Christian
dc.creatorDavis, Marc
dc.creatorNewman, Jeffrey A.
dc.creatorCoil, Alison L.
dc.date2001-09-10
dc.date.accessioned2026-07-07T01:59:55Z
dc.date.available2026-07-07T01:59:55Z
dc.descriptionWe have developed a geometrical method based on 3D Voronoi polyhedra and Delaunay tessellation for identifying and reconstructing clusters of galaxies in the next generation of deep, flux-limited redshift surveys. We here describe this algorithm and tests of it using mock catalogs that simulate the DEEP2/DEIMOS redshift survey, which will begin observations in the Spring of 2002 and will provide a detailed three dimensional map of the large scale structure up to redshift 1.5.
dc.descriptionContribution to "Tracing Cosmic Evolution with Galaxy Clusters" (Sesto 2001), ASP Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0109163
dc.identifierhttp://arxiv.org/abs/astro-ph/0109163
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3305
dc.subjectAstrophysics
dc.title3D Identification and Reconstruction of z~1 Clusters: Prospects for the DEEP2 Redshift Survey
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