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            kdblur2: convolve with the laor2 model shape

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 R–Index)

par2

inner radius (units of GM/c^2)

par3

outer radius (units of GM/c^2)

par4

inclination (degrees)

par5

radius at which emissivity power-law index changes

par6

Emissivity power-law index for radii > par6