All Tables

• Table 1: XMM-Newton spectrum: best fit results for the continuum. See text for details.
• Table 2: XMM-Newton spectrum: best fit results for the emission lines. All EWs are calculated against the soft power law, apart for the iron K lines which are calculated against the hard power law. See text for further details. In the last column, the line fluxes from the Chandra observation are given.