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Open Accesshttps://doi.org/10.1051/0004-6361:20066795
Copy DOI Journal: Astronomy & Astrophysics |  Publication Date: Mar 13, 2007 |
 Citations: 24 |
Affiliation: University of California, San Diego, University of Padua, Osservatorio Astronomico di Padova, Imperial College London, California Institute of Technology, Infrared Processing and Analysis Center, Osservatorio astronomico di Bologna, Cornell University, Instituto de Astrofísica de CanariasContext. 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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