The clustering amplitude of X-ray-selected AGN at z ∼ 0.8: evidence for a 
negative dependence on accretion luminosity

Mountrichas, G.; Georgakakis, A.; Menzel, M.-L.; Fanidakis, N.; Merloni, A.; Liu, Z.; Salvato, M.; Nandra, K.

doi:10.1093/mnras/stw281

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The clustering amplitude of X-ray-selected AGN at z ∼ 0.8: evidence for a negative dependence on accretion luminosity

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Georgakakis, A.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Menzel, M.-L.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4724

Merloni, A.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons79621

Liu, Z.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons24380

Salvato, M.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4879

Nandra, K.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Mountrichas, G., Georgakakis, A., Menzel, M.-L., Fanidakis, N., Merloni, A., Liu, Z., et al. (2016). The clustering amplitude of X-ray-selected AGN at z ∼ 0.8: evidence for a negative dependence on accretion luminosity. Monthly Notices of the Royal Astronomical Society, 457(4), 4195-4204. doi:10.1093/mnras/stw281.

Cite as: https://hdl.handle.net/11858/00-001M-0000-002A-4CD5-0

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