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rdblur: convolve with the diskline model shape

A convolution model to smooth a spectrum by relativistic effects from an accretion disk around a non-rotating black hole. Modified from diskline model (Fabian et al. (1989)) by Andy Fabian and Roderick Johnstone.

par1 Index: power law dependence of emissivity (scales as $R^{par1}$). If this parameter is 10 or greater then the accretion disk emissivity law $(1-\sqrt{6/R})/R^3$ is used.
par2 inner radius (units of $GM/c^2$)
par3 outer radius (units of $GM/c^2$)
par4 inclination (degrees)