Basic properties of Narrow-Line Seyfert 1 Galaxies with Relativistic Jets

L. Foschini , E. Angelakis , G. Bonnoli , V. Braito , A. Caccianiga , L. Fuhrmann , L. Gallo , G. Ghirlanda

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G. Ghisellini D. Grupe T. Hamilton S. Kaufmann S. Komossa Y. Y. Kovalev A. Lahteenmaki M. L. Lister K. Mannheim L. Maraschi S. Mathur B. M. Peterson P. Romano P. Severgnini G. Tagliaferri J. Tammi F. Tavecchio O. Tibolla M. Tornikoski S. Vercellone

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classification 🌌 astro-ph.HE

keywords fermigalaxiesnarrow-linerlnls1ssampleseyfertswiftavailable

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We present the preliminary results of a survey performed with Swift to observe a sample of radio-loud Narrow-Line Seyfert 1 Galaxies (RLNLS1s). Optical-to-X-ray data from Swift are complemented with gamma-ray observations from Fermi/LAT and radio measurements available in the literature. The comparison with a sample of bright Fermi blazars indicates that RLNLS1s seem to be the low-power tail of the distribution.

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Basic properties of Narrow-Line Seyfert 1 Galaxies with Relativistic Jets

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