$\begin{figure} \par\includegraphics[width=7.8cm,clip]{Gi101_fig1.ps}\end{figure}$ Figure 1: XMM-Newton/EPIC image of the bright X-ray transient XMMU J174554.4-285456 close to Sgr A*. Red, green and blue code for photons with energy 0.5-2, 2-5, and 5-10 keV, respectively.
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In the text

$\begin{figure} \par\includegraphics[width=5.5cm,angle=90,clip]{Gi101_fig2.ps}\end{figure}$ Figure 2: XMM-Newton/EPIC background subtracted light curve of XMMU J174554.4-285456 in the 2-10 keV energy band. The lower light curve shows the background level scaled to the source extraction area.
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In the text

$\begin{figure} \par\includegraphics[width=5.5cm,angle=-90,clip]{Gi101_fig3.ps}\end{figure}$ Figure 3: PN spectrum of XMMU J174554.4-285456 with the best fit model using an absorbed power-law continuum (see Table 1) and data-to-model ratio.
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In the text

$\begin{figure} \par\begin{tabular}{cc} \includegraphics[width=6cm,angle=90,clip]... ...s} & \includegraphics[width=8.5cm,clip]{Gi101_fig4r.ps}\end{tabular}\end{figure}$ Figure 4: Timing analysis of XMMU J174554.4-285456 in the 2-10 keV energy band. left: power spectrum of the EPIC 2.6 s-binned light curve. The enlargement shows the X-ray pulsation candidate at the frequency $5.85\pm 0.07$ mHz corresponding to a period of $171\pm 2$ s. right: folded light curve for the period $171.6\pm 0.3$ s found with periodogram analysis.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{Gi101_fig1.ps}\end{figure}$	Figure 1: XMM-Newton/EPIC image of the bright X-ray transient XMMU J174554.4-285456 close to Sgr A*. Red, green and blue code for photons with energy 0.5-2, 2-5, and 5-10 keV, respectively.
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$\begin{figure} \par\includegraphics[width=5.5cm,angle=90,clip]{Gi101_fig2.ps}\end{figure}$	Figure 2: XMM-Newton/EPIC background subtracted light curve of XMMU J174554.4-285456 in the 2-10 keV energy band. The lower light curve shows the background level scaled to the source extraction area.
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$\begin{figure} \par\includegraphics[width=5.5cm,angle=-90,clip]{Gi101_fig3.ps}\end{figure}$	Figure 3: PN spectrum of XMMU J174554.4-285456 with the best fit model using an absorbed power-law continuum (see Table 1) and data-to-model ratio.
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$\begin{figure} \par\begin{tabular}{cc} \includegraphics[width=6cm,angle=90,clip]... ...s} & \includegraphics[width=8.5cm,clip]{Gi101_fig4r.ps}\end{tabular}\end{figure}$	Figure 4: Timing analysis of XMMU J174554.4-285456 in the 2-10 keV energy band. left: power spectrum of the EPIC 2.6 s-binned light curve. The enlargement shows the X-ray pulsation candidate at the frequency $5.85\pm 0.07$ mHz corresponding to a period of $171\pm 2$ s. right: folded light curve for the period $171.6\pm 0.3$ s found with periodogram analysis.
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