Clustering of X-Ray-Selected AGN

Figure 1

Halo bias as function of halo masses for a fixed redshift 𝑧=1 and the corresponding predictions of Press and Shechter [56] (long-dashed line), Sheth and Tormen [57] (dashed line), Sheth et al. [55] (solid line), and Tinker et al. [58] (dotted line).