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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., MNRAS 238, 729) by Andy Fabian and Roderick Johnstone.


Index: power law dependence of emissivity (scales as Rpar1). If this parameter is 10 or greater then the accretion disk emissivity law (1-sqrt(6/R))/R^3 is used.


inner radius (units of GM/c^2)


outer radius (units of GM/c^2)


inclination (degrees)