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 ) |
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 |