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Fig. 15.

image

Left panel: multiplicative bias after full METACALIBRATION as a function of mAUTO for the baseline simulations (black for σw = 2 pixels; lightgrey for σw = 3 pixels) and the grid-based simulations (red points for σw = 2 pixels). Right panel: multiplicative bias after full METACALIBRATION as a function of the input half-light radius (reff) for galaxies with mAUTO. Bottom panels: estimated selection bias from full METACALIBRATION (points). The solid lines show the corresponding direct measurements of the selection bias (cf. Figs. 4 and 5).

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