SINFONI's take on Star Formation, Molecular Gas, and Black Hole Masses   in AGN
  We present some preliminary (half-way) results on our adaptive optics spectroscopic survey of AGN at spatial scales down to 0.085arcsec. Most of the data were obtained with SINFONI which provides integral field capability at a spectral resolution of R~4000. The themes on which we focus in this contribution are: star formation around the AGN, the properties of the molecular gas and its relation to the torus, and the mass of the black hole. 
R. Davies, R. Genzel, L. Tacconi, F. Muller Sanchez, J. Thomas, S.   Friedrich