Rest-frame Near-IR Observations of High-z Galaxy Clusters

Details Rest-frame Near-IR Observations of High-z Galaxy Clusters Rest-frame Near-IR Observations of High-z Galaxy Clusters

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...204.4131s&link_type=abstract

American Astronomical Society Meeting 204, #41.31; Bulletin of the American Astronomical Society, Vol. 36, p.726

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We present early results from a Spitzer Space Telescope program of IRAC imaging of high-z galaxy clusters. These data sample the rest frame near-IR, enabling study of the evolved stellar populations in the member galaxies up to z 4. Combined with ground-based optical and near-IR photometry, the new IRAC observations allow us to estimate the stellar masses of galaxies in clusters over a very large range in redshift.

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