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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. 8.

Projected correlation function for the CLASXS and CDF‐N fields and the combined sample. (a)–(c) Best‐fit parameters, as well as the χ2 contours for the CLASXS+CDF‐N sample, the CLASXS sample, and the CDF‐N sample, respectively. Contour levels are for 1, 2, and 3 σ confidence levels. (d) Projected correlation function for CLASXS (open circles) and CDF‐N (black dots) fields. Lines are the best fit shown in (a)–(c). Solid line, CLASXS+CDF‐N; dotted line, CLASXS; dashed line, CDF‐N.

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