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The Spatial Clustering of ROSAT All-Sky Survey AGNs. I. The Cross-correlation Function with SDSS Luminous Red Galaxies

  • Authors: Mirko Krumpe, Takamitsu Miyaji, and Alison L. Coil

KRUMPE, MIYAJI, & COIL 2010 The Astrophysical Journal 713 558.

  • Provider: AAS Journals

Caption: Figure 8.

Probability contours for the power law normalization r 0 and slope γ of the total RASS-AGN sample (black, central contour), low L X RASS-AGN sample (gray, left contour), and high L X RASS-AGN sample (gray, right contour). The solid contours represent the 1σ confidence intervals (68.3%) for a one-parameter fit based on a correlated χ 2 = χ 2 min + 1.0 (Equation (12)), while the dotted lines illustrate the corresponding intervals for a two-parameter fit (1σ, correlated χ 2 = χ 2 min + 2.3).

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