Left: 0.5−7 keV spectrum of PID 319, obtained from the full exposure of three EPIC cameras. The data are plotted in flux units of EF_E as a function of energy as observed. The energy range corresponds to the rest-frame 0.87−12.2 keV. The small decline at the lowest energies is due to the Galactic absorption. The spectral flattening towards higher energies (see text) can be noticed. Right: details of the Fe K band spectrum plotted in the rest-frame 4−9 keV range. The Fe K line shows a moderately broad profile.