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Caption: Figure 9.
Emissivity profiles associated with the Shakura–Sunyaev accretion disk with a coronal height of 5 rg and Eddington ratios ﹩\dot{M}/{\dot{M}}_{\,\rm{Edd}\,}=0.3﹩, 0.7, 1.1, and 17. Each line corresponds to the respective accretion disk geometry with a different Eddington ratio.
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