Constant density ionised disc model (note that this has been superceded by a new version)These large table model files, provided by David Ballantyne (drb@ast.cam.ac.uk) calculate the reflection spectrum from an ionized slab of an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: Tuesday, 14-Feb-2023 13:32:37 EST |