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Deep X-ray spectroscopy of obscured AGN in the XMM-CDFS

AuthorsVignali, C.; Comastri, A.; Ranalli, P.; Cappelluti, N.; Gilli, R.; Iwasawa, K.; Carrera, Francisco J. CSIC ORCID CVN ; Georgantopoulos, I.; Brusa, M.; Puccetti, S.; Mainieri, V.; Rovilos, E.; Vito, F.; Falocco, Serena CSIC ORCID; Paolillo, M.; Castelló-Mor, N. CSIC; Brunner, H.; Brand, T.; Balestra, I.; Figonuenov, A.
Issue Date2014
CitationX-ray Universe (2014)
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.
DescriptionTrabajo presentado al Symposium the X-ray Universe, celebrado en Dublin (Irlanda) del 16 al 19 de junio de 2014.
Appears in Collections:(IFCA) Comunicaciones congresos
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