All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{0484_f1a.ps}\\ \includegraphics[width=8cm,clip]{0484_f1b.ps} . \end{figure}$ Figure 1: IBIS/ISGRI deconvolved images of the 3EG J1736-2908 sky region: mosaic of the region with exposure of 320 ks, in the energy bands 20-40 ( left) and 40-60 ( right) keV. The 3EG J1736-2908 probability contours at 95% and 99% confidence level are shown. The detected source position inside the probability contours is coincident with the GRANAT source GRS 1734-292 (see text)
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=13cm,clip]{0484_f2.ps} \end{figure}$ Figure 2: Spectral Energy Distribution (SED) of GRS 1734-292. We show here all published data: VLA and ESO (Martí et al. 1998), ASCA (Sakano et al. 2002), ART-P (Pavlinsky et al. 1994), INTEGRAL (present paper), SIGMA (Churazov et al. 1992) and EGRET (Hartman et al. 1999). Infrared and optical data from ESO are corrected with two different absorptions, respectively $1.1\times 10^{22}$ and $2.1\times 10^{22}$ cm^-2. The data include minimum, mean and maximum observed values, in order to show the interval of variation of GRS 1734-292 from non-detection to flares, at different epochs. If not visible, error bars are smaller than size of symbols.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0484_f1a.ps}\\ \includegraphics[width=8cm,clip]{0484_f1b.ps} . \end{figure}$	Figure 1: IBIS/ISGRI deconvolved images of the 3EG J1736-2908 sky region: mosaic of the region with exposure of 320 ks, in the energy bands 20-40 ( left) and 40-60 ( right) keV. The 3EG J1736-2908 probability contours at 95% and 99% confidence level are shown. The detected source position inside the probability contours is coincident with the GRANAT source GRS 1734-292 (see text)
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