The Angular Clustering of Hard X-ray AGNs

Details The Angular Clustering of Hard X-ray AGNs The Angular Clustering of Hard X-ray AGNs

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..424..298k&link_type=abstract

Proceedings of the 9th International Conference of the Hellenic Astronomical Society, proceedings of a conference held 20-24 Sep

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the clustering properties of hard (2-8 keV) X-ray selected sources in CDF-N, CDF-S (fx = 2×10-16 erg s-1 cm-2) and AEGIS (fx = 10-15 erg s-1 cm-2). Modeling the two-correlation function as a power law of the form w(θ) = (θ0/θ)γ-1 we find: (fixing the slope to γ = 1.8) CDF-N θ0 = 1.69±0.2 CDF-S θ0 = 1.69±0.3 AEGIS θ0 = 2.48±0.5. For the sources with spectroscopic redshift available, the clustering lengths appear higher.

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