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The Clustering of AGNs and Galaxies at Intermediate Redshift

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© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation M. J. I. Brown et al 2001 AJ 122 26 DOI 10.1086/321106

1538-3881/122/1/26

Abstract

Galaxies in the environments of 69 0.2 < z < 0.7, UBR-selected active galactic nuclei (AGNs) have been imaged to BJ ∼ 23.5. By applying photometric redshifts and color selection criteria to the galaxy catalog, the AGN-galaxy cross-correlation function has been measured as a function of galaxy type. The spatial cross-correlation of AGNs with red (early-type) galaxies is comparable to the autocorrelation function of elliptical galaxies at low redshift. In contrast, the cross-correlation of AGNs with blue (late-type) galaxies is weak and has been detected with low significance. Since blue galaxies dominate BJ ∼ 23.5 galaxy catalogs, the cross-correlation of UBR-selected AGNs with all galaxies is weak at intermediate redshifts.

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10.1086/321106