Host dark matter halo mass, M_DM, as a function of galaxy stellar mass, M_∗ for the full galaxy sample split by mass and redshift. The WIRDS results are reproduced in all three panels, whilst literature results are added in the centre panel and the galform predictions are added in the right hand panel. In terms of the WIRDS data, the triangles, squares, ×, stars and crosses show the results from the WIRDS data for redshift ranges centred on z = 0.50, z = 0.70, z = 0.90, z = 1.10, z = 1.35 and z = 1.75 respectively. In the centre panel, the thick dashed curve shows the fit to M_DM versus M_⋆ given by Wake et al. (2011) for galaxies at 1 < z < 2 in the NEWFIRM survey, whilst the open circles show the results from Foucaud et al. (2010) at z ≳ 1. In the right hand panel, the predictions from the galform model are given for the same central redshifts.