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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

Journal article published in 2007 by B. Rocca-Volmerange, De Lapparent, N. Seymour ORCID, M. Fioc
This paper was not found in any repository; the policy of its publisher is unknown or unclear.
This paper was not found in any repository; the policy of its publisher is unknown or unclear.

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