Submillimetre galaxies reside in dark matter haloes with masses greater than 3\times10^{11} solar masses

Amblard, Alexandre and Cooray, Asantha and Serra, Paolo and Altieri, B. and Arumugam, V. and Aussel, H. and Blain, A. and Bock, J. and Boselli, A. and Buat, V. and Castro-Rodríguez, N. and Cava, A. and Chanial, P. and Chapin, E. and Clements, D. L. and Conley, A. and Conversi, L. and Dowell, C. D. and Dwek, E. and Eales, S. and Elbaz, D. and Farrah, D. and Franceschini, A. and Gear, W. and Glenn, J. and Griffin, M. and Halpern, M. and Hatziminaoglou, E. and Ibar, E. and Isaak, K. and Ivison, R. J. and Khostovan, A. A. and Lagache, G. and Levenson, L. and Lu, N. and Madden, S. and Maffei, B. and Mainetti, G. and Marchetti, L. and Marsden, G. and Mitchell-Wynne, K. and Nguyen, H. T. and O’Halloran, B. and Oliver, S. J. and Omont, A. and Page, M. J. and Panuzzo, P. and Papageorgiou, A. and Pearson, C. P. and Pérez-Fournon, I. and Pohlen, M. and Rangwala, N. and Roseboom, I. G. and Rowan-Robinson, M. and Portal, M. Sánchez and Schulz, B. and Scott, Douglas and Seymour, N. and Shupe, D. L. and Smith, A. J. and Stevens, J. A. and Symeonidis, M. and Trichas, M. and Tugwell, K. and Vaccari, M. and Valiante, E. and Valtchanov, I. and Vieira, J. D. and Vigroux, L. and Wang, L. and Ward, R. and Wright, G. and Xu, C. K. and Zemcov, M.

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