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PDF Availablehttps://doi.org/10.1051/0004-6361:20066795
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Cite Journal: Astronomy & Astrophysics |  Publication Date: Mar 13, 2007 |
 Citations: 24 |
Affiliation: University of California, San Diego, University of Padua, Osservatorio Astronomico di Padova, Osservatorio astronomico di Bologna, Instituto de Astrofísica de Canarias, California Institute of Technology, Cornell University, Infrared Processing and Analysis Center, Imperial College London
Context. High-redshift ultra luminous infrared galaxies contribute the bulk of the cosmic IR background and are the best candidates for very massive galaxies in formation at .
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