The 2-850 micron SEDs of 170 micron-selected galaxies

Details The 2-850 micron SEDs of 170 micron-selected galaxies The 2-850 micron SEDs of 170 micron-selected galaxies

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.6312s&link_type=abstract

American Astronomical Society Meeting 205, #63.12; Bulletin of the American Astronomical Society, Vol. 36, p.1452

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a detailed 2-850um SED study of a representative sample of the FIRBACK 170um population. These galaxies constitute the brightest ˜ 10% of the contributors to the Cosmic Infrared Background. Their characterization is therefore crucial for constraining galaxy evolution models. Previous studies suggest that the sample spans z ˜ 0-1 and LIR ˜ 1010-1012Lsun. In this paper, we have combined archival Spitzer Space Telescope IRAC and MIPS data with our previous observations including deep K-band imaging, SCUBA, ISO, and VLA. This unprecedented spectral coverage allows us to discuss both the properties of individual sources, and the statistical properties of the sample.

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