The Evolution of Infrared-luminous Galaxies at High Redshift

Details The Evolution of Infrared-luminous Galaxies at High Redshift The Evolution of Infrared-luminous Galaxies at High Redshift

Feb 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sptz.prop..288p&link_type=abstract

Spitzer Proposal ID #288

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Scientific paper

My primary goal is to understand how different populations of infrared-luminous galaxies are related to each other, and how they all fit into our picture of galaxy evolution. This goal will be addressed using upcoming deep, wide-field Spitzer and SCUBA-2 extragalactic surveys, along with multi-wavelength imaging and spectroscopic data. I will use these datasets to constrain the shape of the IR SED to obtain accurate estimates of the star formation rates and dust properties. I will use IRS observations to characterize the mid-IR SED as a function of redshift, luminosity and sample selection to separate AGN and starburst components.

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