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.
|
par1 |
Index: power law dependence of emissivity (scales as R–Index). If this
parameter is 10 or greater then the accretion disk emissivity law |
|
par2 |
inner radius (units of |
|
par3 |
outer radius (units of |
|
par4 |
inclination (degrees) |
is used.