Figure 6 from The Spatial Clustering of ROSAT All-Sky Survey AGNs. I. The Cross-correlation Function with SDSS Luminous Red Galaxies

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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 6.

Projected LRG ACF (boxes), RASS-AGN–LRG CCF (triangles), and the inferred RASS-AGN ACF (diamonds). For all data points, we show the 1σ uncertainties. The obtained best power law fit of the RASS-AGN ACF, using the covariance matrix and fitting over r _p = 0.3–15 h ⁻¹ Mpc, is shown as a dashed line.

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