Galaxy population properties of the massive X-ray luminous galaxy cluster XDCP J0044.0-2033 atz= 1.58

2014/06/18 by R. Fassbender, A. Nastasi, Joana Santos +25
Physics and Astronomy · #Astrophysical Phenomena and Observations #Galaxies: Formation, Evolution, Phenomena #Gamma-ray bursts and supernovae #astro-ph.CO #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201423941

published as A&A 568, A5 (2014) · 23 pages, 19 color figures, accepted for publication in A&A, v2 matches journal version

arxiv created 2014/06/18 · openalex publication_date 2014/06/20 · arxiv updated 2014/09/05 · openalex created_date 2022/10/02 · openalex updated_date 2026/08/05

Abstract

Context. Recent observational progress has enabled the detection of galaxy clusters and groups out to very high redshifts and for the first time allows detailed studies of galaxy population properties in these densest environments in what was formerly known as the “redshift desert” at z> 1.5.

Citations

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