GC rotation velocities (left) and velocity dispersions (right) compared to the stellar body of the galaxies. The stellar rotation amplitudes and velocity dispersions were extracted from the kinematic maps at 1 R_eff where possible. Upper panels: V_GCS and σ_GCS for the total GCS. The colour gives the stellar mass of the host galaxy and the symbols show the galaxy morphology. Bottom panel: values, when only the red or blue GCs were modelled. For galaxies with more than 10 GCs in either population, a dotted line connects the values. The dashed line in all panels gives the one-to-one relation. FCC 213 is not shown because no kinematic map was available.