Over half of the far-infrared background light comes from galaxies at z >or= 1.2.

Devlin, Mark J; Ade, Peter A R; Aretxaga, Itziar; Bock, James J; Chapin, Edward L; Griffin, Matthew; Gundersen, Joshua O; Halpern, Mark; Hargrave, Peter C; Hughes, David H; Klein, Jeff; Marsden, Gaelen; Martin, Peter G; Mauskopf, Philip; Moncelsi, Lorenzo; Netterfield, Calvin B; Ngo, Henry; Olmi, Luca; Pascale, Enzo; Patanchon, Guillaume; Rex, Marie; Scott, Douglas; Semisch, Christopher; Thomas, Nicholas; Truch, Matthew D P; Tucker, Carole; Tucker, Gregory S; Viero, Marco P; Wiebe, Donald V

Devlin, Mark J; Ade, Peter A R; Aretxaga, Itziar; Bock, James J; Chapin, Edward L; Griffin, Matthew; Gundersen, Joshua O; Halpern, Mark; Hargrave, Peter C; Hughes, David H; Klein, Jeff; Marsden, Gaelen; Martin, Peter G; Mauskopf, Philip; Moncelsi, Lorenzo; Netterfield, Calvin B; Ngo, Henry; Olmi, Luca; Pascale, Enzo; Patanchon, Guillaume; Rex, Marie; Scott, Douglas; Semisch, Christopher; Thomas, Nicholas; Truch, Matthew D P; Tucker, Carole; Tucker, Gregory S; Viero, Marco P; Wiebe, Donald V.

Affiliation

Devlin MJ; Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, Pennsylvania 19104, USA. devlin@physics.upenn.edu

Nature ; 458(7239): 737-9, 2009 Apr 09.

Article in En | MEDLINE | ID: mdl-19360081

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Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Nature Year: 2009 Document type: Article Affiliation country: United States Country of publication: United kingdom

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