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

2001/09/10 by Christian Marinoni, C. Marinoni, M. Davis +9
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #Gamma-ray bursts and supernovae #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0109163

Contribution to "Tracing Cosmic Evolution with Galaxy Clusters" (Sesto 2001), ASP Conference Series

arxiv created 2001/09/10 · openalex publication_date 2001/09/10 · arxiv updated 2009/12/01 · openalex created_date 2025/10/24 · openalex updated_date 2026/07/28

Abstract

We have developed a geometrical method based on 3D Voronoi polyhedra and\nDelaunay tessellation for identifying and reconstructing clusters of galaxies\nin the next generation of deep, flux-limited redshift surveys. We here describe\nthis algorithm and tests of it using mock catalogs that simulate the\nDEEP2/DEIMOS redshift survey, which will begin observations in the Spring of\n2002 and will provide a detailed three dimensional map of the large scale\nstructure up to redshift 1.5.\n

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