Constant density ionised disc models
These large table model files, provided by David Ballantyne (firstname.lastname@example.org) 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
HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/Public
Last modified: Monday, 28-Dec-2020 10:22:58 EST