All Tables

Table 1: Spectral fit components to the (0.3-10) keV energy band. The individual Cols. 2 to 8 refer to the spectral components applied in the fit. The rows specify the measured values. The broad-band spectral energy distribution measured with these components is shown in Fig. 7. The foreground absorption has been fixed to the Galactic value. ^aNote: for the first three components the normalization is given in units of [ $10^{-14} / (4 \pi (D_{\rm A} (1+{\rm z}))^2) \int n_{\rm e}~ n_{\rm H}~ {\rm dV}$ ], where $D\rm _A$ is the angular size distance to the source (cm), $n\rm _e$ is the electron density ( $\rm cm^{-3})$ , and $\rm n_H$ is the hydrogen density ( $\rm cm^{-3}$ ). For the last five components the normalization is given in units of [ $\rm 10^{-5}~photons\ cm^{-2}\ s^{-1}\ keV^{-1}$ ] at 1 keV. The fluxes and luminosities are absorption corrected.