Comparison between the observed NIFS velocity dispersion map and three representative Schwarzschild models, all at the same M/L = 1.80 and with different black hole masses. From left to right: the data, the formal best fit M_BH (using LOESS) model, a model with M_BH a factor of five higher than the previous one (70% higher than the derived upper limit), and the model with M_BH for which the sphere of influence is the same as our spatial resolution. The M_BH values are given above the maps. Note the appearance of the central velocity dispersion peak for models above the formal upper limit. The same comparison is given for the JAM V_rms models in the lower panels.