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.
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par1 |
Index: power law dependence of emissivity (scales as R–par1) |
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par2 |
inner radius (units of |
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par3 |
outer radius (units of |
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par4 |
inclination (degrees) |
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par5 |
radius at which emissivity power-law index changes |
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par6 |
Emissivity power-law index for radii > par6 |
