The extragalactic background light at far-infrared wavelengths comes from optically faint, dusty, star-forming galaxies with star formation rates at the level of a few hundred solar masses per year. These faint submillimetre galaxies are challenging to study individually, but their average properties can be studied using statistics such as the angular power spectrum of the background intensity variations. This study reports excess clustering over the linear prediction at arcminute angular scales in the power spectrum of brightness fluctuations at 250, 350 and 500 micrometres. It is found that submillimetre galaxies are located in dark matter haloes with a minimum mass of log10[Mmin/solar mass]=11.5+0.7-0.2 at 350° micrometres.
- Alexandre Amblard
- Asantha Cooray
- M. Zemcov
