An ultra-deep Spitzer look at the most distant galaxy cluster

Computer Science

Scientific paper

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Scientific paper

We propose to obtain very deep IRAC imaging in the 3.6 and 4.5 micron passbands on the recently discovered Cl J1449+0856, the most distant galaxy cluster to date, at z=2.07. This very distant cluster is different from z>2 proto-clusters in that it shows both an X-ray emission and a significant population of quiescent galaxies, suggesting an evolved state despite its high redshift. It thus offers a unique opportunity of studying galaxy evolution in overdense environments at early cosmic times. The proposed observations will probe for the first time the rest-frame near-infrared emission of faint cluster galaxies at z~2, allowing us to determine the stellar mass function at a cosmic epoch which is thought to be critical for witnessing ongoing stellar mass assembly in cluster galaxies. These data will be a crucial counterpart of the already available deep HST NICMOS and WFC3 photometry in identifying cluster members. Moreover, the deep rest-frame near-infrared photometry will be a fundamental tool in disentangling the red cluster galaxy population in its two components of truly quiescent objects and heavily reddened star forming sources. The proposed observations will thus allow us to take full advantage of the unique discovery of Cl J1449+0856 to test different scenarios for the evolution of cluster galaxies at a still unprobed epoch.

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