Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10 11 solar masses
- Amblard, Alexandre
- Cooray, Asantha
- Serra, Paolo
- Altieri, B.
- Arumugam, V.
- Aussel, H.
- Blain, A.
- Bock, J.
- Boselli, A.
- Buat, V.
- Castro-Rodríguez, N.
- Cava, A.
- Chanial, P.
- Chapin, E.
- L. Clements, D.
- Conley, A.
- Conversi, L.
- D. 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.
- J. Ivison, R.
- A. Khostovan, A.
- Lagache, Guilaine
- Levenson, L.
- Lu, N.
- Madden, S.
- Maffei, B.
- Mainetti, G.
- Marchetti, L.
- Marsden, G.
- Mitchell-Wynne, K.
- T. Nguyen, H.
- O'Halloran, B.
- J. Oliver, S.
- Omont, A.
- J. Page, M.
- Panuzzo, P.
- Papageorgiou, A.
- P. Pearson, C.
- Pérez-Fournon, I.
- Pohlen, M.
- Rangwala, N.
- G. Roseboom, I.
- Rowan-Robinson, M.
- Sánchez Portal, M.
- Schulz, B.
- Scott, Douglas
- Seymour, N.
- L. Shupe, D.
- J. Smith, A.
- A. Stevens, J.
- Symeonidis, M.
- Trichas, M.
- Tugwell, K.
- Vaccari, M.
- Valiante, E.
- Valtchanov, I.
- D. Vieira, J.
- Vigroux, L.
- Wang, L.
- Ward, R.
- Wright, Gavin
- K. Xu, C.
- Zemcov, M.
DOIAbstract
International audienceThe extragalactic background light at far-infrared wavelengths comes from optically faint, dusty, star-forming galaxies in the Universe with star formation rates of a few hundred solar masses per year. These faint, submillimetre galaxies are challenging to study individually because of the relatively poor spatial resolution of far-infrared telescopes. Instead, their average properties can be studied using statistics such as the angular power spectrum of the background intensity variations. A previous attempt at measuring this power spectrum resulted in the suggestion that the clustering amplitude is below the level computed with a simple ansatz based on a halo model. Here we report excess clustering over the linear pre...
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