$\begin{figure} \par\includegraphics[width=4.5cm,clip]{7536fig1.ps} \end{figure}$ Figure 1: XMMU J174716.1-281048/IGR J17464-2811 observed with IBIS/ISGRI between 20 and 25 keV. The image has been collected in 63 s during the X-ray burst.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=5.75cm]{7536fig2.ps} \includegraphics[... ...=5.65cm]{7536fig3.ps} \includegraphics[width=5.65cm]{7536fig4.ps} \end{figure}$ Figure 2: From the top to bottom: JEM-X1 (3-6 keV), JEM-X1 (6-10 keV) and ISGRI (18-26 keV) lightcurves including the type-I X-ray burst from IGR J17464-2811(binsize = 3 s). The INTEGRAL persistent flux is consistent with zero.
Open with DEXTER

In the text

$\begin{figure} { \hbox{\hspace{0.5cm} \includegraphics[height=7.2cm,angle=-90]{7... ...ace{.6cm} \includegraphics[height=7.2cm,angle=-90]{7536fig6.ps} }}\end{figure}$ Figure 3: Combined IBIS/ISGRI and JEM-X1 photons spectra and model (black-body) of the burst detected by INTEGRAL (left); spectrum of the persistent emission of XMMU J174716.1-281048 fitted with a simple absorbed power-law (EPIC/PN camera observation) is shown (right).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=0,height=8.1cm]{7536fig7.eps} \end{figure}$ Figure 4: X-ray images (0.5-10 keV) of the source field obtained with the EPIC-PN camera in 2000 (on the left) and in 2003 (on the right). The transient XMMU J174716.1-281048 is clearly evident in the centre of the 2003 image. The circle (1' radius) marks the uncertainty region of the burst observed with JEM-X.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=0,height=5.0cm]{7536fig8.ps} \end{figure}$ Figure 5: Long term X-ray lightcurve of XMMU J174716.1-281048. The two observations performed with XMM-Newton in 2003 and 2005 are marked with squares, while meaningful upper limits are reported with arrows. The persistent flux (2-10 keV) is corrected for the absorption. Uncertainties on fluxes are smaller than symbols used.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=4.5cm,clip]{7536fig1.ps} \end{figure}$	Figure 1: XMMU J174716.1-281048/IGR J17464-2811 observed with IBIS/ISGRI between 20 and 25 keV. The image has been collected in 63 s during the X-ray burst.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=5.75cm]{7536fig2.ps} \includegraphics[... ...=5.65cm]{7536fig3.ps} \includegraphics[width=5.65cm]{7536fig4.ps} \end{figure}$	Figure 2: From the top to bottom: JEM-X1 (3-6 keV), JEM-X1 (6-10 keV) and ISGRI (18-26 keV) lightcurves including the type-I X-ray burst from IGR J17464-2811(binsize = 3 s). The INTEGRAL persistent flux is consistent with zero.
Open with DEXTER

$\begin{figure} { \hbox{\hspace{0.5cm} \includegraphics[height=7.2cm,angle=-90]{7... ...ace{.6cm} \includegraphics[height=7.2cm,angle=-90]{7536fig6.ps} }}\end{figure}$	Figure 3: Combined IBIS/ISGRI and JEM-X1 photons spectra and model (black-body) of the burst detected by INTEGRAL (left); spectrum of the persistent emission of XMMU J174716.1-281048 fitted with a simple absorbed power-law (EPIC/PN camera observation) is shown (right).
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=0,height=8.1cm]{7536fig7.eps} \end{figure}$	Figure 4: X-ray images (0.5-10 keV) of the source field obtained with the EPIC-PN camera in 2000 (on the left) and in 2003 (on the right). The transient XMMU J174716.1-281048 is clearly evident in the centre of the 2003 image. The circle (1' radius) marks the uncertainty region of the burst observed with JEM-X.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=0,height=5.0cm]{7536fig8.ps} \end{figure}$	Figure 5: Long term X-ray lightcurve of XMMU J174716.1-281048. The two observations performed with XMM-Newton in 2003 and 2005 are marked with squares, while meaningful upper limits are reported with arrows. The persistent flux (2-10 keV) is corrected for the absorption. Uncertainties on fluxes are smaller than symbols used.
Open with DEXTER