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We present some preliminary (half-way) results on our adaptive opticsspectroscopic survey of AGN at spatial scales down to 0.085arcsec. Most of thedata were obtained with SINFONI which provides integral field capability at aspectral resolution of R~4000. The themes on which we focus in thiscontribution are: star formation around the AGN, the properties of themolecular gas and its relation to the torus, and the mass of the black hole.Comment: 5 pages, 2 figures. To appear in Science Perspectives for 3D  Spectroscopy. ESO Astrophysics Symposia. Ed by M. Kissler-Patig, M. Roth and  J. Wals

SINFONI’s take on Star Formation, Molecular Gas, and Black Hole Masses in AGN