The luminosity-dependent clustering of Hα emitters from z~0.8 to z~2.2 with HiZELS

Poster presented at the conference Galaxy evoltion Across Time, 12-16 June, Paris, France

We study the clustering of star-forming galaxies, using halo models to derive dark matter halo masses. Typical galaxies in our samples are star-forming centrals, residing in host halos of mass 10^12 M_solar. We find strong trends between galaxy Hα luminosity and dark matter halo mass at all redshifts.

See also https://arxiv.org/abs/1704.05472