BeppoSAX observations of Narrow-Line Seyfert 1 galaxies: II. Ionized   iron features in Arakelian 564
  The BeppoSAX observations of the bright Narrow-Line Seyfert 1 galaxy Ark 564 are presented along with a high quality optical spectrum taken at the 1.5m telescope at La Silla. The 0.1-10 keV X-ray spectrum is characterized by a strong soft component which is best described by blackbody-like emission with a temperature of about 160 eV. At higher energies a steep (Gamma = 2.4) power-law tail is present. There is evidence of an ionized reflector in the form of an iron line and edge. We do not find significant evidence of soft X-ray features if the spectrum is modelled with a two component continuum. The optical and X-ray spectral properties support the hypothesis of a high accretion rate onto a low mass black hole. 
A.Comastri, G.M. Stirpe, C. Vignali, W.N. Brandt, K.M. Leighly, F.   Fiore, M. Guainazzi, G. Matt, F. Nicastro, E.M. Puchnar...