Illustration of GC extraction from MUSE data of FCC 167. Top panel: residual image obtained by subtractingthe IMFIT surface-brightness model of FCC 167 from the galaxy surface-brightness distribution extracted from MUSE data. The GC candidates from MUSE data (blue circles) and GCs in the HST/ACS GC catalogue (Jordán et al. 2015; red crosses) are shown. Middle panel: map of the mean stellar velocity of FCC 167 shown in Fig. 8 and radial velocities of the GCs. Bottom panel: spectra of two MUSE GCs with S∕N ≈ 25 (purple line) and 5 (green line) whose location is indicated in the top panel by the filled purple and open green triangles, respectively.