A new (2+1)D cluster finding algorithm based on photometric redshifts: large scale structure in the Chandra deep field south

2006/11/29 by D. Trevese, Dario Trevese, M. Castellano +5
Physics and Astronomy · #Astronomy and Astrophysical Research #Chandra Deep Field South #Cluster (spacecraft) #Cluster analysis #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Photometric redshift #Redshift #Scale (ratio) #Scientific Research and Discoveries #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065384

10 pages, 9 figures, accepted for publication in A&A

arxiv created 2006/11/29 · openalex publication_date 2006/12/18 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims.We study galaxy clustering and explore the dependence of galaxy properties on the the environment up to a redshift z ~ 1, on the basis of a deep multi-band survey in the Chandra Deep Field South.

Citations

• The structural and scaling properties of nearby galaxy clusters
• TheB‐Band Luminosity Function of Red and Blue Galaxies up toz= 3.5
• Environment and Galaxy Evolution at Intermediate Redshift in the CNOC2 Survey
• The K20 survey. I. Disentangling old and dusty star-forming galaxies in the ERO population
• Large-Scale Structure in the Universe Indicated by Galaxy Clusters

Cited by

• A comprehensive study of large-scale structures in the GOODS-SOUTH field up to \mathsf z ∼ 2.5