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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 4.

Same as Figure 3, but for the opposite orientation of the caustic, i.e., for ﹩{\theta }_{{\rm{c}}}=270^\circ ﹩. Note that the amplification patterns are independent of the direction of the movement of the caustic. The magnification patterns of Figures 3 and 4 could both run from the left to the right or vice versa.

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