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XMM-Newton Surveys of the Canada-France Redshift Survey Fields - III: The Environments of X-ray Selected AGN at 0.4<z<0.6

T. J. Waskett·S. A. Eales·W. K. Gear·H. J. McCracken·S. Lilly·M. Brodwin
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Abstract

The environmental properties of a sample of 31 hard X-ray selected AGN are investigated, from scales of 500 kpc down to 30 kpc, and are compared to a control sample of inactive galaxies. The AGN all lie in the redshift range 0.4 =0 clusters. It is suggested that minor mergers with low mass companions is a likely candidate for the mechanism by which these modest luminosity AGN are fuelled.

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T. J. Waskett, S. A. Eales, W. K. Gear, H. J. McCracken, S. Lilly, M. Brodwin. 2005-08-03. XMM-Newton Surveys of the Canada-France Redshift Survey Fields - III: The Environments of X-ray Selected AGN at 0.4<z<0.6. https://doi.org/10.1111/j.1365-2966.2005.09480.x

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