Best-fitting Schwarzschild model of FCC 47. Top row: Voronoi binned kinematic data for FCC 47. Left to right: surface brightness, radial velocity and velocity dispersion. Middle row: best-fit Schwarzschild model. Bottom row: residuals created by subtracting the model from the data. The white patches indicate masked bins. The surface brightness counters are taken from the MGE model (see also Fig. B.1). The plotting ranges are not identical to those shown in Fig. 5.