reflect: reflection from neutral material
Convolution model for reflection from neutral material according to the method of Magdziarz & Zdziarski (1995, MNRAS, 273, 837). This is a generalization of the pexrav and bexrav models. When using this model it is essential to extend the energy range over which the model is calculated because photons at higher energies are Compton downscattered into the target energy range. The energy range can be extended using the extend command. The upper limit on the energies should be set above that for which the input spectrum has significant flux. See the help on pexrav or bexrav for further information and admonitions.
par1 |
reflection scaling factor (1 for isotropic source above disk) |
par2 = z |
redshift |
par3 |
abundance of elements heavier than He relative to the solar abundances |
par4 |
iron abundance relative to the above |
par5 |
cos i, the inclination angle |