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XMM‐Newton Observations of the Narrow‐Line Seyfert 1 Galaxy Mrk 335 in a Historical Low X‐Ray Flux State

  • Authors: Dirk Grupe, Stefanie Komossa, Luigi C. Gallo, Andrew C. Fabian, Josefin Larsson, Anil K. Pradhan, Dawei Xu, and Giovanni Miniutti

Grupe et al. 2008 The Astrophysical Journal 681 982.

  • Provider: AAS Journals

Caption: Fig. 4.

XMM‐Newton EPIC pn 0.3–12.0 keV (black) and MOS 0.3–10.0 keV (red+green) spectra of Mrk 335 fitted with a broken power law with ﹩\alpha _{\mathrm{X}\,,\mathrm{soft}\,}=1.89﹩, ﹩\alpha _{\mathrm{X}\,,\mathrm{hard}\,}=-0.19﹩, ﹩E_{\mathrm{break}\,}=1.73﹩ keV as listed in Table 5. The absorption column density is fixed to the Galactic value (﹩3.96\times 10^{20}﹩ cm−2; Dickey & Lockman 1990).

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