XMM-Newton Survey of a Distance-limited Sample of Seyfert Galaxies: Preliminary Spectral Results

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dc.creatorCappi, M.
dc.creatorDi Cocco, G.
dc.creatorPanessa, F.
dc.creatorBassani, L.
dc.creatorCaroli, E.
dc.creatorDadina, M.
dc.creatorComastri, A.
dc.creatorDella Ceca, R.
dc.creatorFilippenko, A. V.
dc.creatorFoschini, L.
dc.creatorGianotti, F.
dc.creatorHo, L. C.
dc.creatorMakishima, K.
dc.creatorMalaguti, G.
dc.creatorMulchaey, J. S.
dc.creatorPalumbo, G. G. C.
dc.creatorPiconcelli, E.
dc.creatorSargent, W. L. W.
dc.creatorStephen, J.
dc.creatorTrifoglio, M.
dc.creatorWeaver, K.
dc.creatorZamorani, G.
dc.date2003-03-17
dc.date.accessioned2026-07-07T02:07:59Z
dc.date.available2026-07-07T02:07:59Z
dc.descriptionAn unbiased estimate of the average intrinsic X-ray properties and column density distribution of Seyfert galaxies in the local Universe is crucial to validate unified models of active galactic nuclei (AGNs) and to synthesis models for the X-ray background. We present here preliminary results obtained from an on-going XMM-Newton study (~250 ks awarded in the EPIC GT) on a well-defined, statistically complete, and significant sample of nearby Seyfert galaxies.
dc.description4 pages, 3 figures, to appear in "Carnegie Observatories Astrophysics Series, Vol. 1: Coevolution of Black Holes and Galaxies," ed. L. C. Ho (Pasadena: Carnegie Observatories, http://www.ociw.edu/ociw/symposia/series/symposium1/proceedings.html)'
dc.identifierhttps://arxiv.org/abs/astro-ph/0303367
dc.identifierhttp://arxiv.org/abs/astro-ph/0303367
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5878
dc.subjectAstrophysics
dc.titleXMM-Newton Survey of a Distance-limited Sample of Seyfert Galaxies: Preliminary Spectral Results
dc.typetext

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