Fig. 14.

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Galaxy (projected) circular velocity profiles used here: the solid lines correspond to the results from MGEFit, each one with its respective model indicated in the legend; the dashed lines are Keplerian profiles as originated from a SMBH with masses of 3.22 × 109 M⊙ (red line) and 4.33 × 109 M⊙ (blue line); the vertical dotted lines are (from left to right) the ALMA pixel size (), HST/WFC3 pixel size (
), and CO disk size (∼5″).
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