FERO (Finding Extreme Relativistic Objects): statistics of relativistic broad Fe K alpha lines in AGN

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dc.creatorLonginotti, A. L.
dc.creatorde La Calle, I.
dc.creatorBianchi, S.
dc.creatorGuainazzi, M.
dc.creatorDovciak, M.
dc.date2007-09-20
dc.date2007-10-04
dc.date.accessioned2026-07-07T08:33:58Z
dc.date.available2026-07-07T08:33:58Z
dc.descriptionThe properties of the relativistically broadened Fe K alpha line emitted in Active Galactic Nuclei (AGN) are still debated among the AGN community. Recent works seem to exclude that the broad Fe line is a common feature of AGN. The analysis of a large sample composed by 157 XMM-Newton archival observations of radio quiet AGN is presented here. This ongoing project is a development of the work reported in Guainazzi et al. 2006.
dc.descriptionProceeding of "The nuclear region, host galaxy and environment of active galaxies", symposium for the 60th birthday of Deborah Dultzin-Hacyan, held in Huatulco April 18-20, 2007; version with typos corrected
dc.identifierhttps://arxiv.org/abs/0709.3268
dc.identifierhttp://arxiv.org/abs/0709.3268
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/139276
dc.subjectAstrophysics
dc.titleFERO (Finding Extreme Relativistic Objects): statistics of relativistic broad Fe K alpha lines in AGN
dc.typetext

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