Fig. 3 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. 3.

Probability of source detection as a function of off‐axis angle and 2–8 keV fluxes. Contour levels are 0.1, 0.3, 0.5, 0.7, 0.9, 0.95, and 0.99. Top panels, soft band; bottom panels, hard band. Left panels, 70 ks exposures; right panels, 40 ks exposures.

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