Galaxy Clusters at 0.9<z<1.7 in the AKARI NEP deep field

Details Galaxy Clusters at 0.9<z<1.7 in the AKARI NEP deep field Galaxy Clusters at 0.9<z<1.7 in the AKARI NEP deep field

2008-10-02

arxiv.org/abs/0810.0529v2

Astronomy and Astrophysics

Astrophysics

Accepted for publication in PASJ AKARI special issue. Full-resolution version available at http://ifa.hawaii.edu/~tomo/resea

Scientific paper

There is a huge gap between properties of red-sequence selected massive galaxy clusters at z<1 and Lyman-break selected proto-clusters at z>3. It is important to understand when and how the z>3 proto-clusters evolve into passive clusters at z<1. We aim to fill this cluster desert by using the space-based N4(4um) imaging with the AKARI. The z'-N4 color is a powerful separator of cluster galaxies at z>1, taking advantage of the 4000A break and the 1.6um bump. We carefully selected 16 promising cluster candidates at 0.9

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