HEASoft and XSPEC are now available as conda packages. See details ....
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.
Note that due to the energy binning the convolution process can produce spurious structures around sharp features in the spectrum being convolved. We strongly recommend testing for this by using the energies command to change the binning.
par1 | Index: power law dependence of emissivity (scales as |
par2 | inner radius (units of |
par3 | outer radius (units of |
par4 | inclination (degrees) |