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Photometric redshifts as a tool for studying the Coma cluster galaxy populations

2008/09/11 by C. Adami, O. Ilbert, R. Pello +7
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Galaxies: Formation, Evolution, Phenomena #astro-ph

paper · pdf · doi:10.1051/0004-6361:200809845

14 pages, 2 figures in jpeg format, accepted in A&A

arxiv created 2008/09/11 · openalex publication_date 2008/10/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31

Abstract

Aims. We apply photometric redshift techniques to an investigation of the Coma cluster galaxy luminosity function (GLF) at faint magnitudes, in particular in the u* band where basically no studies are presently available at these magnitudes.

Citations