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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 (Laor 1991http://adsabs.harvard.edu/abs/1991ApJ...376...90L). 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 ) |

par4 |
inclination (degrees) |

par5 |
radius at which emissivity power-law index changes |

par6 |
Emissivity power-law index for radii >par6 |