I will describe the results of a recent study 
of SEDs of a sample of AGN, and the new model used fit these
observations. Using these data we are able to determine 
the black hole spins in some cases. Further out from the nucleus we 
have begun to model the ionising and heating effects of the SEDs
on the dusty molecular torus. I will compare our preliminary model 
results with observations of highly ionised emission line species, and 
also the near infrared lines of [FeII] and molecular hydrogen formed deep 
within the torus, and which provides new insights into its physical properties.