A convolution model to smooth a spectrum by relativistic effects from an accretion disk around a rotating black hole. Uses Ari Laor's calculation including GR effects (Laor 1991). Modified from laor model by Andy Fabian and Roderick Johnstone.
|par1||Index: power law dependence of emissivity (scales as )|
|par2||inner radius (units of )|
|par3||outer radius (units of )|