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
(2006). 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.
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 |
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 |
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Last modified: Friday, 23-Aug-2024 13:20:40 EDT
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