Figure 9 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 9.

Distribution of spectral peaks for three lamppost corona heights ﹩h=5\,{r}_{{\rm{g}}}﹩ (solid line), ﹩h=10\,{r}_{{\rm{g}}}﹩ (dashed line), and ﹩h=100\,{r}_{{\rm{g}}}﹩ (dotted line) (﹩a=0.9﹩, ﹩i=82\buildrel{\circ}\over{.} 5﹩, ﹩\beta =0.5﹩).

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