Best fit halo mass as a function of mean stellar mass. The red squares (blue triangles) denote the early-type (late-type) galaxies. The separation of the lenses into early/late-types is based on their brightness profiles. The dashed lines are the powerlaw fits, with values as indicated in the text. For stellar masses lower than 10¹¹ M_⊙ the best fit halo masses of early- and late-type galaxies are similar, but for M_∗ > 10¹¹ M_⊙ we find that the best fit halo masses of early-types are greater.