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We present 0.5 -160 micron Spectral Energy Distributions (SEDs) of galaxies,detected at 70microns with the Multiband Imaging Photometer for Spitzer (MIPS),using broadband imaging data from Spitzer and ground-based telescopes.Spectroscopic redshifts, in the range 0.2<z<1.5, have been measured as part ofthe Deep Extragalactic Evolutionary Probe2 (DEEP2) project. Based on the SEDswe explore the nature and physical properties of the sources. Using the opticalspectra we derive Hbeta and [OII]-based Star Formation Rates (SFR) which are10-100 times lower than SFR estimates based on IR and radio. The median offsetin SFR between optical and IR is reduced by a factor of ~3 when we apply atypical extinction corrections. We investigate mid-to-far infrared correlationsfor low redshift (>0.5) and high redshift (0.5<z<1.2) bins. Using this unique``far-infrared'' selected sample we derive an empirical mid to far-infraredrelationship that can be used to estimate the infrared energy budget ofgalaxies in the high-redshift universe. Our sample can be used as a template totranslate far-infrared luminosities into bolometric luminosities for highredshift objects

AEGIS: Infrared Spectral Energy Distributions of MIPS 70 μm-selected Sources