Trend of the fraction of potential contaminants as a function of the magnitude of the galaxy. The top panel uses a radius of 0.̋5 to search for contaminants, the middle panel 1.̋0, and the bottom panel 1.̋5. The downturn at faint magnitudes with the smallest search radii is a reflection of the lower redshift completeness. The solid blue line shows the level when we consider only objects we were able to deblend with MUSE. The dashed green line shows the result if only galaxies for which |(z_MUSE−pz) / (1 + z_MUSE)| < 0.15 are kept.