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<i>SPITZER</i>- AND<i>HERSCHEL</i>-BASED SPECTRAL ENERGY DISTRIBUTIONS OF 24 μm BRIGHT<i>z</i>∼ 0.3-3.0 STARBURSTS AND OBSCURED QUASARS
In this paper, we characterize the infrared spectral energy distributions (SEDs) of mid-IR-selected z ∼ 0.3–3.0 and LIR ∼ 1011–1013 L☉ galaxies, and study how their SEDs differ from those of local and high-z analogs. Infrared SEDs depend both on the power source (AGN or star formation) and the dust …