All Tables

• Table 1: The log of all analysed observations, and exposure times. Values in brackets show net exposure times after filtering for particle induced flares.
• Table 2: The total flux (2-10 keV) as measured adopting the baseline model (described further in the text).
• Table 3: Best fit parameters for the baseline model applied to the six observations.
• Table 4: Fluxes and equivalent widths for the broad line component after the flux of the narrow line component has been fixed to the weighted mean value. Note that BeppoSAX and Chandra measured fluxes are no longer only upper limits.