All Figures

$\begin{figure} \par\includegraphics[width=12.2cm,clip]{7734fig1.ps}\end{figure}$ Figure 1: IBIS-ISGRI mosaic image constructed on the basis of the 715 science windows (FCFOV) between 20 and 60 keV. The point sources detected in the field of view are individually pointed out. The large structures centered on Cyg X-1 are artificial. The coordinate grid specifies the right ascension and the declination.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{7734fig2.ps}\end{figure}$ Figure 2: Fraction of the IBIS-ISGRI mosaic image between 20 and 60 keV (see Fig. 1). The position of our main targets is specified. The bright source on this image is Cyg X-3. The coordinate grid specifies the right ascension and the declination.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=12.2cm,clip]{7734fig1.ps}\end{figure}$	Figure 1: IBIS-ISGRI mosaic image constructed on the basis of the 715 science windows (FCFOV) between 20 and 60 keV. The point sources detected in the field of view are individually pointed out. The large structures centered on Cyg X-1 are artificial. The coordinate grid specifies the right ascension and the declination.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{7734fig2.ps}\end{figure}$	Figure 2: Fraction of the IBIS-ISGRI mosaic image between 20 and 60 keV (see Fig. 1). The position of our main targets is specified. The bright source on this image is Cyg X-3. The coordinate grid specifies the right ascension and the declination.
Open with DEXTER