Multi-wavelength study of a sample of nearby Seyfert galaxies

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dc.creatorPanessa, F.
dc.creatorBassani, L.
dc.creatorCappi, M.
dc.creatorDadina, M.
dc.creatorIwasawa, K.
dc.date2004-10-04
dc.date.accessioned2026-07-07T02:14:53Z
dc.date.available2026-07-07T02:14:53Z
dc.descriptionOne of the least biased complete Seyfert sample available to date has been considered to perform an X-ray survey using the capabilities of XMM-Newton and Chandra satellites. The X-ray nuclear luminosities obtained have been used to perform a multi-wavelength analysis as a powerfull tool in the identification of heavily obscured objects. The new X-ray data, together with highest quality nuclear fluxes available from the radio to the optical band, allow us to obtain nuclear Spectral Energy Distributions (SEDs) for type 1 and type 2 objects in our sample. The results obtained from the analysis of the SED have been discussed in the framework of Unified Models.
dc.description8 pages, 8 figures. Proceedings of the VI Italian Conference on Active Galactic Nuclei. See http://www.arcetri.astro.it/~agn6/proceedings/
dc.identifierhttps://arxiv.org/abs/astro-ph/0410083
dc.identifierhttp://arxiv.org/abs/astro-ph/0410083
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8304
dc.subjectAstrophysics
dc.titleMulti-wavelength study of a sample of nearby Seyfert galaxies
dc.typetext

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