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We measure the angular correlation function, w(theta), from 0.5 to 30arcminutes of detected sources in two wide fields of the Herschel Multi-tieredExtragalactic Survey (HerMES). Our measurements are consistent with theexpected clustering shape from a population of sources that trace the darkmatter density field, including non-linear clustering at arcminute angularscales arising from multiple sources that occupy the same dark matter halos. Bymaking use of the halo model to connect the spatial clustering of sources tothe dark matter halo distribution, we estimate source bias and halo occupationnumber for dusty sub-mm galaxies at z ~ 2. We find that sub-mm galaxies with250 micron flux densities above 30 mJy reside in dark matter halos with massabove (5\pm4) x 10^12 M_sun, while (14\pm8)% of such sources appear assatellites in more massive halos.

HerMES: Halo Occupation Number and Bias Properties of Dusty Galaxies from Angular Clustering Measurements