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The Obscuration of COSMOS AGN

Ezequiel TREISTER
(IfA, Hawaii)

I will present a study of the near and mid-IR properties of X-ray selected AGN, both from XMM and Chandra, in the COSMOS field. I will focus in a comparison with dust re-emission models in order to determine physical and geometrical parameters of the obscuring material. I will further discuss possible trends with AGN parameters like luminosity and redshift.


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