Revealing Physical Nature of Infrared Luminous Galaxies at 0.3<z<2.7 Using HST and Spitzer

Details Revealing Physical Nature of Infrared Luminous Galaxies at 0.3<z<2.7 Using HST and Spitzer Revealing Physical Nature of Infrared Luminous Galaxies at 0.3<z<2.7 Using HST and Spitzer

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sptz.prop40025y&link_type=abstract

Spitzer Proposal ID #40025

Physics

Scientific paper

We aim to determine physical properties of IR luminous galaxies at 0.3 0.8mJy and their mid-IR spectra have already provided the majority targets with spectroscopic redshifts (0.31 ULIRGs, as in the local Universe. (2) study the co-evolution of star formation and blackhole accretion by investigating the relations between the fraction of starburst/AGN measured from mid-IR spectra vs. HST morphologies, L(bol) and z. (3) obtain the current best estimates of the far-IR emission, thus L(bol) for this sample, and establish if the relative contribtuion of mid-to-far IR dust emission is correlated with morphology.

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