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Fig. 8


Comparison between the observed NIFS velocity dispersion map and three low MBH Schwarzschild models, all at the same M/L = 1.80. From left to right: the data, the model with the lowest MBH used in this work, a model which is formally outside the three-sigma uncertainty level, and the formal best fit model from Fig. 7left panel. The MBH values are given above the maps. There are no significant differences between these three models, and the differences with the data are on the level of systematics, arguing that the three-sigma uncertainty level on the left hand panel of Fig. 7 should be continuous and no lower limit to the MBH is found in NGC 4414.

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