pexmon: neutral Compton reflection with self-consistent Fe and Ni lines.
This model from Nandra et al. (2007)
combines pexrav
with self-consistently generated Fe K, Fe K
, Ni
K
and the Fe K
Compton shoulder. Line strengths are based on Monte Carlo calculations
by George & Fabian (1991)
which are parametrized for
by :
with inclination dependence for degrees :
and abundance dependence :
The Fe K and Ni K
line fluxes are 11.3% and 5%
respectively of that for Fe K
. The Fe K
Compton shoulder is
approximated as a gaussian with E = 6.315 keV and
keV. The
inclination dependence is taken from Matt (2002)
such
that :
The model parameters are :
par1 | |
par2 | |
par3 | scale, the scaling factor for reflection; <0 = no direct component, 1 = isotropic source above the disk |
par4 | |
par5 | |
par6 | |
par7 | the inclination angle (degrees). |
norm | normalization is the photon flux at 1 keV
(photons/keV/cm |