Fig. A.1
Ratio of the best fit halo mass for the unscattered lens catalogue to the best fit halo mass for the lenses to which a log-normal scatter of 0.1 in stellar mass has been applied, for the early-type galaxies (left) and the late-type galaxies (right). The halo masses are underestimated at the high stellar mass end due to low mass objects scattering into the high mass bins.
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