Infrared Observations of AGN
  We present results from an imaging and spectroscopic study of the dust properties of Seyfert galaxies in the 1-10um range. The data are compared to state of the art models of torus emission to constrain geometrical and physical properties of the obscuring medium. 
P. Lira, F. Marin, L. Videla, A. Alonso-Herrero, D.M. Alexander & M.   Ward