Investigated merger-sensitive parameters as functions of the rotational support (vertical axis in each tile) and the M_JAM mass of the galaxy (horizontal axis in each tile). Each point represents one galaxy. The colors of the points indicate the values of the quantities stated in the tiles of the figures, coded according to the color bars given to the right of each tile. For shells, streams, tails, disturbed isophotes, and dust lanes, the values of zero, one, or two indicate that the feature is not present, is likely present, or is certainly present, respectively. The frequency of shells, streams, and tails indicates the number of these features in the galaxy. For KDCs, CRCs, KTs, and the 2σ features, the values of zero or one mean that the kinematic substructure is not or is present in the galaxy, respectively.