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Fig. 1


Four different SEDs that we used for our photoionisation balance calculations in Cloudy, SPEX, and XSTAR. The AGN1 and AGN2 SEDs are the normal and obscured SED versions of a typical Seyfert AGN (NGC 5548), taken from Mehdipour et al. (2015). The PL SED is a power-law continuum with Γ = 2, and the BB SED is a black body with T = 50 eV.

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