Fig. F.1.
Comparison between symmetrized kinematic data and best-fitting Schwarzschild models for the galaxies NGC 584, NGC 2784, and NGC 3640. For each galaxy we show the SINFONI data on the left side and the large-scale data on the right side. The panels are ordered as follows: From left to right: mean velocity, velocity dispersion, and h3 and h4 Gauss-Hermite moments. From top to bottom: symmetrized data, model for the best-fitting parameters from Table 5, and residual map defined as difference between the Schwarzschild model and observed kinematics divided by the observational errors.
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