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Fig. 15.

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Bias on lens mass properties as a function of the minimum Einstein radius. First panel: median log αsps. Dotted lines indicate values of αsps corresponding to a Chabrier and a Salpeter IMF (αsps = 1 corresponds to a Kroupa IMF). Second panel: median Mh at log = 11.4. Third panel: median MDM, 5 at log = 11.4 and log Re = 1.2. Fourth panel: median γDM at log = 11.4 and log Re = 1.2. In each panel, the dashed line indicates the value of the parent population. Error bars indicate the standard deviation of the mean of the lens sample.

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