X-ray eclipse tomography: Resolving the extent of X-ray-emitting region(s) in the Seyfert galaxy ESO 362-G18

Open Access

Fig. 8.

Evolution of the covering fraction towards the soft excess (red) and hot corona (blue). Black circles denote $C_{f}^{(SE)} = C_{f}^{(HC)}$ $Mathematical equation: $ C_{\mathrm{f}}^{\mathrm{(SE)}} = C_{\mathrm{f}}^{\mathrm{(HC)}} $$ . We also show flat-top Gaussian model-examples fitted to the C_f evolution of both components; see the main text for details.

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