The Origin of Massive Galaxies in High Redshift Clusters

Details The Origin of Massive Galaxies in High Redshift Clusters The Origin of Massive Galaxies in High Redshift Clusters

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sptz.prop50050f&link_type=abstract

Spitzer Proposal ID #50050

Physics

Scientific paper

We propose to obtain IRS 16 um peak-up imaging of 15 well-studied, Spitzer-selected, massive galaxy clusters at 1.1 < z < 1.4. These observations will provide mid-IR photometry for 200-300 cluster members, including a minimum of 40 spectroscopically confirmed cluster members. In combination with 24 um data awarded in cycle GO-3, these data will allow us to identify and study those IR luminous cluster galaxies powered primarily by star formation. Together with extensive, ongoing z > 1 spectroscopy and ground- and space-based multiwavelength imaging, these 16 um data will allow us to measure the contribution of cluster ULIRGs and LIRGs to the buildup of stellar mass in the Universe.

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