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dc.contributor.authorVignali, C.-
dc.contributor.authorComastri, A.-
dc.contributor.authorRanalli, P.-
dc.contributor.authorCappelluti, N.-
dc.contributor.authorGilli, R.-
dc.contributor.authorIwasawa, K.-
dc.contributor.authorCarrera, Francisco J.-
dc.contributor.authorGeorgantopoulos, I.-
dc.contributor.authorBrusa, M.-
dc.contributor.authorPuccetti, S.-
dc.contributor.authorMainieri, V.-
dc.contributor.authorRovilos, E.-
dc.contributor.authorVito, F.-
dc.contributor.authorFalocco, Serena-
dc.contributor.authorPaolillo, M.-
dc.contributor.authorCastelló-Mor, N.-
dc.contributor.authorBrunner, H.-
dc.contributor.authorBrand, T.-
dc.contributor.authorBalestra, I.-
dc.contributor.authorFigonuenov, A.-
dc.date.accessioned2018-09-27T12:02:34Z-
dc.date.available2018-09-27T12:02:34Z-
dc.date.issued2014-
dc.identifier.citationX-ray Universe (2014)-
dc.identifier.urihttp://hdl.handle.net/10261/170303-
dc.descriptionTrabajo presentado al Symposium the X-ray Universe, celebrado en Dublin (Irlanda) del 16 al 19 de junio de 2014.-
dc.description.abstractXMM-CDFS survey: -X-ray spectroscopy allows for a proper spectral characterization of >100 AGN in the XMM-CDFS, up to high redshifts. -The number of Compton-thick AGN is in fairly good agreement with XRB model expectations. Still need to analyze the faint AGN population (but poorer photon statistics and much lower snr). -X-rays are a good tracer of obscured accretion. Deep X-ray survey strategy is the way to go, but combined mid-IR/optical selection may help picking up the obscured AGN population.-
dc.relation.isversionofPublisher's version-
dc.rightsopenAccess-
dc.titleDeep X-ray spectroscopy of obscured AGN in the XMM-CDFS-
dc.typepresentación-
dc.date.updated2018-09-27T12:02:34Z-
dc.description.versionPeer Reviewed-
dc.language.rfc3066eng-
dc.relation.csic-
Appears in Collections:(IFCA) Comunicaciones congresos
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