Submillimetre galaxies reside in dark matter haloes with masses greater than 3 x 10(11) solar masses

Record Type

  • Journal Articles

Full Title

  • Submillimetre galaxies reside in dark matter haloes with masses greater than 3 x 10(11) solar masses

Author(s)

  • Amblard A, Cooray A, Serra P, Altieri B, Arumugam V, Aussel H, Blain A, Bock J, Boselli A, Buat V, Castro-Rodriguez N, Cava A, Chanial P, Chapin E, Clements D, Conley A, Conversi L, Dowell C, Dwek E, Eales S, Elbaz D, Farrah D, Franceschini A, Gear W, Glenn J, Griffin M, Halpern M, Hatziminaoglou E, Ibar E, Isaak K, Ivison R, Khostovan A, Lagache G, Levenson L, Lu N, Madden S, Maffei B, Mainetti G, Marchetti L, Marsden G, Mitchell-Wynne K, Nguyen H, O'Halloran B, Oliver S, Omont A, Page M, Panuzzo P, Papageorgiou A, Pearson C, Perez-Fournon I, Pohlen M, Rangwala N, Roseboom I, Rowan-Robinson M, Sanchez Portal M, Schulz B, Scott D, Seymour N, Shupe D, Smith A, Stevens J, Symeonidis M, Trichas M, Tugwell K, Vaccari M, Valiante E, Valtchanov I, Vieira J, Vigroux L, Wang L, Ward R, Wright G, Xu C, Zemcov M

Publication Title

Publication Title (abbreviated)

  • NATURE

Publication Date

  • 2011 Feb 24

DOI

  • 10.1038/nature09771

ISSN

  • 0028-0836

Volume

  • 470

Issue

  • 7335

Page Count

  • 3

First Page

  • 510

Last Page

  • 512

Keyword(s)

Citation

  • Amblard A, Cooray A, Serra P, Altieri B, Arumugam V, Aussel H, Blain A, Bock J, Boselli A, Buat V, et al. Submillimetre galaxies reside in dark matter haloes with masses greater than 3 x 10(11) solar masses. NATURE. 2011;470 (7335):510-512.

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