A convolution model to smooth a spectrum by relativistic effects from an accretion disk around a rotating black hole. The accretion disk has a broken-power law emissivity profile. Uses Ari Laor's calculation including GR effects (ApJ 376, 90). Modified from laor2 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 )|
|par5||radius at which emissivity power-law index changes|
|par6||Emissivity power-law index for radii >par6|