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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 14.

Distribution of (from top to bottom) reconstructed black hole spin, accretion disk inclination, corona height, and β-parameter for simulated data sets with 40 measured microlensed energy spectra for the input values ﹩{P}_{0}\,=\{{a}_{0}=0.8,i=77\buildrel{\circ}\over{.} 5,h=10\,{r}_{{\rm{g}}},\beta =0.5\}﹩.

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