Multi-wavelength study of a sample of nearby Seyfert galaxies

Details Multi-wavelength study of a sample of nearby Seyfert galaxies Multi-wavelength study of a sample of nearby Seyfert galaxies

2004-10-04

arxiv.org/abs/astro-ph/0410083v1

Astronomy and Astrophysics

Astrophysics

8 pages, 8 figures. Proceedings of the VI Italian Conference on Active Galactic Nuclei. See http://www.arcetri.astro.it/~agn6/

Scientific paper

One 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.

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