A Census of LIRGs in Clusters of Galaxies in the First Half of the Universe from the IRAC Shallow Survey

Details A Census of LIRGs in Clusters of Galaxies in the First Half of the Universe from the IRAC Shallow Survey A Census of LIRGs in Clusters of Galaxies in the First Half of the Universe from the IRAC Shallow Survey

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006hst..prop11002e&link_type=abstract

HST Proposal ID #11002. Cycle 15

Physics

Scientific paper

The incidence of LIRGs and ULIRGs is roughly two orders of magnitude higher in the field at redshift z > 1, and at these redshifts such objects dominate the global star formation activity. Mergers which fuel such activity might be expected to enhance the frequency of LIRGs in dense environments. We propose to use MIPS to obtain a census of LIRGs in z > 1 galaxy clusters from a well defined sample found in the IRAC Shallow Survey. Supporting IRAC and HST ACS data are also requested.

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