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The XMM-Newton wide field survey in the COSMOS field: redshift evolution of AGN bias and subdominant role of mergers in triggering moderate luminosity AGN at redshift up to 2.2

MPS-Authors
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Allevato,  V.
Office of the Director (DI), Max Planck Institute for Plasma Physics, Max Planck Society;
Group 'Astrophysics and Laboratory Plasma Studies' (ALPS), Max Planck Institute for Plasma Physics, Max Planck Society;

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Hasinger,  G.
Group 'Astrophysics and Laboratory Plasma Studies' (ALPS), Max Planck Institute for Plasma Physics, Max Planck Society;
Office of the Director (DI), Max Planck Institute for Plasma Physics, Max Planck Society;

/persons/resource/persons110314

Salvato,  M.
Group 'Astrophysics and Laboratory Plasma Studies' (ALPS), Max Planck Institute for Plasma Physics, Max Planck Society;
Office of the Director (DI), Max Planck Institute for Plasma Physics, Max Planck Society;

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Allevato, V., Finoguenov, A., Cappelluti, N., Miyaji, T., Hasinger, G., Salvato, M., et al. (2011). The XMM-Newton wide field survey in the COSMOS field: redshift evolution of AGN bias and subdominant role of mergers in triggering moderate luminosity AGN at redshift up to 2.2. The Astrophysical Journal, 736(2): 99 (15pp). doi:10.1088/0004-637X/736/2/99.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0026-EB62-1
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