Astronomy and Astrophysics – Astronomy
Scientific paper
May 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aas...212.8802m&link_type=abstract
American Astronomical Society, AAS Meeting #212, #88.02; Bulletin of the American Astronomical Society, Vol. 40, p.267
Astronomy and Astrophysics
Astronomy
Scientific paper
The bolometric luminosities of high-redshift submillimeter-selected ultraluminous infrared galaxies (ULIRGs) are dominated by thermal emission from dust at infrared wavelengths. In order to properly understand the distribution of dust within such high-redshift ULIRGs, and to determine the luminosity function of the population as a whole, we therefore must acquire a sampling of their complete infrared spectral energy distributions (SEDs). Here, we present MIPS 70 and 160 micron and SHARC-II 350 micron images of a sample of high-redshift submillimeter-selected ULIRGs located behind lensing clusters of galaxies. We use this data, in combination with deep SCUBA 850 micron images, to construct rest-frame mid-infrared to submillimeter SEDs.
Borys Colin
Dowell Charles (Darren)
Egami Eiichi E.
Marshall Andrew J.
Zemcov Michael
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