The evolution of the cluster optical galaxy luminosity function betweenz= 0.4 and 0.9 in the DAFT/FADA survey

2014/12/18 by N. Martinet, Nicolas Martinet, Florence Durret +16 · 25 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Cluster (spacecraft) #Computer science #Context (archaeology) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Gamma-ray bursts and supernovae #Geography #Luminosity #Luminosity function #Physics #Redshift #astro-ph.CO #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201423796

published in Astronomy and Astrophysics 575, A116 (EDP Sciences) · accepted for publication in A&A

arxiv created 2014/12/18 · openalex publication_date 2015/03/01 · arxiv updated 2015/03/11 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. There is some disagreement about the abundance of faint galaxies in high-redshift clusters, with contradictory results in the literature arising from studies of the optical galaxy luminosity function (GLF) for small cluster samples.

Citations

• Evolution sincez= 1 of the Morphology‐Density Relation for Galaxies
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• Morphological Transformation from Galaxy Harassment
• galics- VI. Modelling hierarchical galaxy formation in clusters
• Photometric redshifts as a tool for studying the Coma cluster galaxy populations
• Down-sizing in galaxy formation atz∼ 1 in the Subaru/XMM-NewtonDeep Survey (SXDS)
• Spatial variations of the optical galaxy luminosity functions and red sequences in the Coma cluster: clues to its assembly history
• Galaxy stellar mass functions of different morphological types in clusters, and their evolution between z= 0.8 and 0
• The Evolution of the Star Formation Activity in Galaxies and Its Dependence on Environment