Fraction of galaxies with a given tidal feature (first three panels), any of the three tidal feature types (fourth panel), or a combination of multiple different types of features (fifth panel), f_feat, in three stellar mass bins for Magneticum, MATLAS (Bílek et al. 2020), and for brightest cluster galaxies (BCGs) from Tal et al. (2009) and Kluge et al. (2020). The masses for MATLAS galaxies are taken from the dynamical masses obtained by Cappellari et al. (2013), which roughly correspond to the stellar masses. The vertical lines indicate the 1σ uncertainties.