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–Index) |
par2 |
inner radius (units of ) |
par3 |
outer radius (units of ) |
par4 |
inclination (degrees) |