The broad-band properties of the XMM-Newton Bright Serendipitous Sources

Simple item page
dc.creatorDella Ceca, R.
dc.creatorMaccacaro, T.
dc.creatorCaccianiga, A.
dc.creatorSevergnini, P.
dc.creatorBraito, V.
dc.date2004-07-07
dc.date.accessioned2026-07-07T02:13:45Z
dc.date.available2026-07-07T02:13:45Z
dc.descriptionWe present here "The XMM-Newton Bright Serendipitous Survey", a survey program conducted by the XMM-Newton Survey Science Center. In particular we discuss the main goals of this project, we present the sample(s) and the current optical breakdown and we discuss some broad band spectral properties as derived from an hardness ratio analysis of the single sources. Finally we report the 4.5--7.5 keV Log(N$>$S)-LogS for type 1 and type 2 AGN.
dc.descriptionOn Behalf of the XMM-Newton Survey Science Centre (SSC) Consortium, 6 pages, 3 figures, Presented at the 48th meeting of the Italian Astronomical Society, Milan, April 19-23, 2004. To appear in the Proceedings
dc.identifierhttps://arxiv.org/abs/astro-ph/0407127
dc.identifierhttp://arxiv.org/abs/astro-ph/0407127
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7921
dc.subjectAstrophysics
dc.titleThe broad-band properties of the XMM-Newton Bright Serendipitous Sources
dc.typetext

Files

Collections

arXiv