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Rocca-Volmerange, B. and de Lapparent, V. and Seymour, N. et al. (2007) The 12 μm ISO-ESO-Sculptor and 24 μm Spitzer faint counts reveal a population of ULIRGs as dusty massive ellipticals: Evolution by types and cosmic star formation. Astronomy and Astrophysics, 475 (3). pp. 801-812. ISSN 0004-6361. http://resolver.caltech.edu/CaltechAUTHORS:20100223-111955718