Left panel: multiplicative bias after full METACALIBRATION for galaxies with 20 < m_AUTO < 24.5 as a function of the separation to the nearest galaxy with m_input < 26 in the input catalogue (top) and selection bias (bottom) for a weight function with σ_w = 2 pixels (black) and σ_w = 3 pixels (grey). Right panel: idem, but now as a function of distance to the nearest detected galaxy. The insets in the panels zoom in on the results for separations larger than 2″. The solid lines in the bottom panels show the corresponding direct measurements of the selection bias.