Fig. 11.
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Comparison of the estimated enclosed mass profile for NGC 4550 resulting from the Gauss Hermite (orange) and non-parametric (blue) stellar kinematics binned to different S/N. The thin lines show the result of the respective best-fit models seen so far with S/N = 60; the thick lines (and shaded uncertainty) show the results of the kinematic data binned to S/N = 150.
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