next up previous contents
Next: Lsmooth Up: Convolution Model Components Previous: Kdblur2

kerrconv: accretion disk line shape with BH spin as free parameter

Convolves the current spectrum with the line shape from the kerrdisk model. A detailed description can be found in Brenneman & Reynolds (2006ApJ...652.1028B). This model is quite slow so is best used after models such as laor or diskline have been employed to get an estimate of the best-fit parameters.

 

 par1   =  emissivity index for the inner disk

 par2   =  emissivity index for the outer disk

 par3   =  break radius separating the inner and outer portions of the disk (gravitational radii)

 par4   =  dimensionless black hole spin

 par5   =  disk inclination angle to the line of sight (degrees)

 par6   =  inner radius of the disk  in units of the radius of marginal stability

 par7   =  outer radius of the disk  in units of the radius of marginal stability

 



next up previous contents
Next: Lsmooth Up: Convolution Model Components Previous: Kdblur2