All Figures

$\begin{figure} \par\includegraphics[height=9.5cm,width=8cm,clip]{Fe261_fig1.ps} \end{figure}$ Figure 1: EPIC light curves (MOS 1+MOS 2+PN) and hardness ratio (HR) within a radius of 10 $^{\prime \prime }$ around Sgr A* position. The time binning is 100 s, and the error bars indicate 1 $\sigma$ uncertainties. Upper panel: The 2-10 keV light curve shows the quiescent and the flare periods. Middle panel: The 2-5 keV and 5-10 keV light curves during the flare period. Lower panel: quiescent subtracted HR during the flare period. Long dashed line: mean HR value, and short dashed lines: 1 $\sigma$ error bars.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{Fe261_fig2.ps} \end{figure}$ Figure 2: EPIC spectra of the flare, within a radius of 10 $^{\prime \prime }$ around Sgr A* position. The spectrum for the quiescent period is used as background. A power-law model has been fitted taking into account ISM absorption and dust scattering. See Table 1 for parameter fit values.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{Fe261_fig2.ps} \end{figure}$	Figure 2: EPIC spectra of the flare, within a radius of 10 $^{\prime \prime }$ around Sgr A* position. The spectrum for the quiescent period is used as background. A power-law model has been fitted taking into account ISM absorption and dust scattering. See Table 1 for parameter fit values.
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