$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{ms3545_fig1t.eps... ...2mm} \includegraphics[angle=-90,width=8.8cm,clip]{ms3545_fig1b.eps} \end{figure}$ Figure 1: The 2-10 keV light curve of 1E 1743-2843 measured with XMM-Newton PN detector after background subtraction. Top panel: time binning of 500 s. Bottom panel: time binning of 100 s.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{ms3545_fig2.ps} \end{figure}$ Figure 2: The 2-12 keV PN spectrum of 1E 1743.1-2843 (binning at 15 $\sigma$ ) and the best-fit power-law continuum model. The lower panel shows the residuals of the data to the model.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{ms3545_fig3.ps} \end{figure}$ Figure 3: Photon index spectra of 1E 1743.1-2843. Filled circles: present XMM-Newton observation (power-law model). Diamonds: average spectrum obtained with ART-P during Fall 1990 (Pavlinsky et al. 1994).
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{ms3545_fig1t.eps... ...2mm} \includegraphics[angle=-90,width=8.8cm,clip]{ms3545_fig1b.eps} \end{figure}$	Figure 1: The 2-10 keV light curve of 1E 1743-2843 measured with XMM-Newton PN detector after background subtraction. Top panel: time binning of 500 s. Bottom panel: time binning of 100 s.
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$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{ms3545_fig2.ps} \end{figure}$	Figure 2: The 2-12 keV PN spectrum of 1E 1743.1-2843 (binning at 15 $\sigma$ ) and the best-fit power-law continuum model. The lower panel shows the residuals of the data to the model.
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$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{ms3545_fig3.ps} \end{figure}$	Figure 3: Photon index spectra of 1E 1743.1-2843. Filled circles: present XMM-Newton observation (power-law model). Diamonds: average spectrum obtained with ART-P during Fall 1990 (Pavlinsky et al. 1994).
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