X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56

Open Access

Fig. 9.

Slices of the simulated eFEDS sensitive area cube. Left: sensitive area for fixed Γ = 2 as a function of L_{2 − 10 keV} and z. Right: sensitive area as a function of Γ and L_{2 − 10 keV} for fixed redshift z = 6. The dotted white (solid black) line shows the parameter configurations at 50% (5%) of the normalised sensitive area.

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