The properties of the ionized gas in the NLS1 Mkn 335

Details The properties of the ionized gas in the NLS1 Mkn 335 The properties of the ionized gas in the NLS1 Mkn 335

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008xmm..prop...12g&link_type=abstract

XMM-Newton Proposal ID #06005402

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Mkn 335, Mkn 335

Scientific paper

We propose a triggered ToO observation of the Narrow-Line Seyfert 1 galaxy Mkn 335 in its low X-ray flux state for 200 ks with XMM-Newton. Mkn 335 is a very bright NLS1 with an exceptional broad iron line. In 2007 we caught it in an extreme low X-ray flux state. Still bright enough in its low-state, it offeres a unique opportunity to distinguish between two AGN key spectral models, the partial covering absorber versus reflection models, and to study the 'warm' circumnuclear BLR gas with the RGS in detail. These studies can only be done in an extreme low-state.

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