$\begin{figure} \par\includegraphics[width=6.9cm,clip]{integral33_f2.eps}\end{figure}$ Figure 2: Image in galactic coordinates of the last pointing of revolution 25 in the 20-40 keV energy band. The detection significance of KS 1947+300 is $11\sigma$ .
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In the text

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{integral33_f3.ps}\end{figure}$ Figure 3: Cyg X-1 count rate spectrum (exposure 00260002) normalized to that of the Crab. The good time interval amounts to roughly 3700 s.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{figure1.eps}\end{figure}$	Figure 1: Scheme of the GPS performed during revolution 26 starting from $l=73^\circ$ .
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$\begin{figure} \par\includegraphics[width=6.9cm,clip]{integral33_f2.eps}\end{figure}$	Figure 2: Image in galactic coordinates of the last pointing of revolution 25 in the 20-40 keV energy band. The detection significance of KS 1947+300 is $11\sigma$ .
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$\begin{figure} \par\includegraphics[width=6.8cm,clip]{integral33_f3.ps}\end{figure}$	Figure 3: Cyg X-1 count rate spectrum (exposure 00260002) normalized to that of the Crab. The good time interval amounts to roughly 3700 s.
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$\begin{figure} \par\includegraphics[height=6.4cm,width=15cm,clip]{integral33_f4.eps}\end{figure}$	Figure 4: Mosaic of 20-40 keV images of all exposures in Table 2.
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