Spatial Correlation Function of the Chandra Selected Active Galactic Nuclei

Details Spatial Correlation Function of the Chandra Selected Active Galactic Nuclei Spatial Correlation Function of the Chandra Selected Active Galactic Nuclei

2006-01-27

arxiv.org/abs/astro-ph/0601634v2

Astrophys.J. 645 (2006) 68-82

Astronomy and Astrophysics

Astrophysics

ApJ accepted. A missing hubble constant h has been noticed in one of the equations and hence corrected. Tables, figures affect

Scientific paper

10.1086/502706

We present the spatial correlation function analysis of non-stellar X-ray point sources in the Chandra Large Area Synoptic X-ray Survey of Lockman Hole Northwest (CLASXS). Our 9 ACIS-I fields cover a contiguous solid angle of 0.4 deg^2 and reach a depth of 3x10^-15 c.g.s in the 2-8 keV band. We supplement our analysis with data from the Chandra Deep Field North (CDFN). The addition of this field allows better probe of the correlation function at small scales. A total of 233 and 252 sources with spectroscopic information are used in the study of the CLASXS and CDFN fields respectively. We calculate both redshift-space and projected correlation functions in comoving coordinates, averaged over the redshift range of 0.1

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