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AEGIS: Infrared Spectral Energy Distributions of MIPS 70micron selected sources

M. Symeonidis·D. Rigopoulou·J. -S. Huang·M. Davis·M. L. N. Ashby·P. Barmby·E. Egami·G. G. Fazio·E. LeFloc'h·G. Rieke·S. P. Willner·G. Wilson
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Abstract

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 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-infrared relationship that can be used to estimate the infrared energy budget of galaxies in the high-redshift universe. Our sample can be used as a template to translate far-infrared luminosities into bolometric luminosities for high redshift objects.

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M. Symeonidis, D. Rigopoulou, J. -S. Huang, M. Davis, M. L. N. Ashby, P. Barmby, E. Egami, G. G. Fazio, E. LeFloc'h, G. Rieke, S. P. Willner, G. Wilson. 2006-11-23. AEGIS: Infrared Spectral Energy Distributions of MIPS 70micron selected sources. https://doi.org/10.1086/517928

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