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arXiv · 1307.1592

Deep Luminosity Functions and Colour-Magnitude Relations for Cluster Galaxies at 0.2 < z < 0.6

R. De Propris·S. Phillipps·M. Bremer
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Abstract

We derive deep $I$ band luminosity functions and colour-magnitude diagrams from HST imaging for eleven $0.2 0.4$ that are not encountered locally. Surface brightness selection effects preferentially influence the detectability of faint red galaxies, accounting for claims of evolution at the faint end.

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R. De Propris, S. Phillipps, M. Bremer. 2013-07-05. Deep Luminosity Functions and Colour-Magnitude Relations for Cluster Galaxies at 0.2 < z < 0.6. https://doi.org/10.1093/mnras%2Fstt1262

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