next up previous contents
Next: kdblur2: convolve with the Up: Convolution Model Components Previous: ireflect: reflection from ionized


kdblur: convolve with the laor model shape

A convolution model to smooth a spectrum by relativistic effects from an accretion disk around a rotating black hole. Uses Ari Laor's calculation including GR effects (ApJ 376, 90). Modified from laor model by Andy Fabian and Roderick Johnstone.

par1 Index: power law dependence of emissivity (scales as $R^{-par1}$)
par2 inner radius (units of $GM/c^2$)
par3 outer radius (units of $GM/c^2$)
par4 inclination (degrees)