All Tables

• Table 1: Results of modeling the BeppoSAX-NFI and XMM-Newton spectra (last entry) with a combination of a disk black body model (Mitsuda et al. 1984; Makishima et al. 1986), Comptonization of soft photons in a hot plasma (Titarchuk 1991), and a narrow emission line.
• Table 2: Summary of the twelve Galactic center observation campaigns of the WFCs. Shown are the time frames of the campaigns, the number of observations, the net exposure time and the number of bursts seen from SAX J1747.0-2853.