The Bright Side of the Hard X-ray Sky: The XMM-Newton Bright Survey

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dc.creatorDella Ceca, R.
dc.creatorCaccianiga, A.
dc.creatorSevergnini, P.
dc.creatorMaccacaro, T.
dc.creatorCocchia, F.
dc.creatorBraito, V.
dc.date2005-10-31
dc.date.accessioned2026-07-07T06:44:06Z
dc.date.available2026-07-07T06:44:06Z
dc.descriptionWe discuss here the main goals and some interesting results of the "XMM-Newton Bright Serendipitous Survey", a research program conducted by the XMM-Newton Survey Science Center in two complementary energy bands (0.5-4.5 keV and 4.5-7.5 keV) in the bright (>~7E-14) flux regime. The very high identification rate (96%) for the X-ray source sample selected in the 4.5-7.5 keV band is used here to have, in this energy range, an "unbiased" view of the extragalactic hard X-ray sky at bright fluxes.
dc.description6 pages, 3 figures, proceedings of the conference "The X-ray Universe 2005", held in San Lorenzo de El Escorial, Spain, 26-30 September 2005, organized by the European Space Astronomy Centre (ESAC) of ESA
dc.identifierhttps://arxiv.org/abs/astro-ph/0510845
dc.identifierhttp://arxiv.org/abs/astro-ph/0510845
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/102667
dc.subjectAstrophysics
dc.titleThe Bright Side of the Hard X-ray Sky: The XMM-Newton Bright Survey
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