Linking X-ray AGN with dark matter halos: a model compatible with AGN luminosity function and large-scale clustering properties

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Fig. 9

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Analog of Fig. 2 with two additional parameters, c₈ ≡ σ and c₉ ≡ α, representing the scatter parameter in the lognormal distribution and the power law index for the L_X-dependent f_duty, respectively. For comparison the contours from Fig. 8 are shown with dashed lines.

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