Figure 6 from Simulations of the Fe Kα Energy Spectra from Gravitationally Microlensed Quasars

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Simulations of the Fe Kα Energy Spectra from Gravitationally Microlensed Quasars

Authors: H. Krawczynski and G. Chartas

2017 The Astrophysical Journal 843 118.

Provider: AAS Journals

Caption: Figure 6.

Top panel: spectral peak energies for black hole spins ﹩a=0﹩ (solid line), ﹩a=0.5﹩ (dashed line), and ﹩a=0.998﹩ (dotted line). Bottom panel: spectral peak energies as a function of a. Both panels: ﹩i=82\buildrel{\circ}\over{.} 5﹩, ﹩h=5\,{r}_{{\rm{g}}}﹩, ﹩\beta =0.5﹩.

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