Constant density ionised disc models
These large table model files, provided by David Ballantyne (ballanty -at- cita.utoronto.ca) calculate the reflection spectrum from an ionized slab of an input power-law. The models include lines and edges from Fe, O, Si, Mg, N and C. They are valid over the energy range 1eV -> 100 keV. Note that these models to not include any relativistic blurring due to proximity to a black hole. These should be added using a separate convolution model if relevant.
These table model files are an updated version with N vi-vii added, increased spectral resolution, and the ability to test variations in the Fe abundance. The old version of this page is available.
See also the reflion model.
Keith Arnaud, Lab. for High Energy Astrophysics, NASA/Goddard Space Flight Center
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