Constant density ionised disc models
These large table model files, provided by David Ballantyne (email@example.com) calculate the reflection spectrum from an ionized slab of an input power-law. The models include lines and edges from Fe, O, Si, Mg, and C. They are valid over the energy range 1eV -> 100 keV. The problem that prevented convergence on some parts of the grid has been fixed in these tables.
Keith Arnaud, Lab. for High Energy Astrophysics, NASA/Goddard Space Flight Center
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Last modified: Thursday, 16-Sep-2004 20:21:53 EDT