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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. 6.

Top: Redshift‐space correlation function for CLASXS field with ﹩3\ \mathrm{Mpc}\,< s< 200﹩ Mpc. Bottom: Maximum likelihood contour for the single power‐law fit. Contour levels are ﹩\Delta S=2.3﹩, 6.17, and 11.8, corresponding to 1, 2, and 3 σ confidence levels for two parameter fits.

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