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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 5.

Top panel: spectral peak energies for inclinations of ﹩12\buildrel{\circ}\over{.} 5﹩ (solid line) and ﹩82\buildrel{\circ}\over{.} 5﹩ (dashed line) for all simulated caustic crossing angles and caustic offsets. Bottom panel: spectral peak energies as a function of inclination i (the box size is proportional to the number of simulated events). Both panels: ﹩a=0.5﹩, ﹩h=5\,{r}_{{\rm{g}}}﹩, ﹩\beta =0.5﹩.

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