Fig. 18 from Spatial Correlation Function of the Chandra‐selected Active Galactic Nuclei

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Spatial Correlation Function of the Chandra‐selected Active Galactic Nuclei

Authors: Y. Yang, R. F. Mushotzky, A. J. Barger, and L. L. Cowie

Yang et al. 2006 The Astrophysical Journal 645 68.

Provider: AAS Journals

Caption: Fig. 18.

(a) Bias evolution. The symbols have the same meaning as in Fig. 16. The solid line is the best fit from C05. The dash‐dotted line shows the linear bias evolution model. (b) Mass of host halo of the X‐ray sources corresponding to the bias in (a).

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