$\begin{figure} \par\psfig{figure=INTEGRAL61_fig1.eps,width=6.7cm,angle=0} \end{figure}$ Figure 1: An image of Cygnus X-1 obtained by using double and triple events. The energy range is 100-700 keV, but most of the events are >300 keV. Contours are at intervals of 4 $\sigma$ ; dashed lines are negative. The peak corresponds to 29 $\sigma$ .
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In the text

$\begin{figure} \psfig{figure=INTEGRAL61_fig2.eps,width=6.7cm,angle=0} \end{figure}$ Figure 2: As Fig. 1 for single events. Note that the intensity scale is not the same: contour intervals are 14 $\sigma$ and the peak is 134 $\sigma$ .
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In the text

$\begin{figure} \par\psfig{figure=INTEGRAL61_fig1.eps,width=6.7cm,angle=0} \end{figure}$	Figure 1: An image of Cygnus X-1 obtained by using double and triple events. The energy range is 100-700 keV, but most of the events are >300 keV. Contours are at intervals of 4 $\sigma$ ; dashed lines are negative. The peak corresponds to 29 $\sigma$ .
Open with DEXTER

$\begin{figure} \psfig{figure=INTEGRAL61_fig2.eps,width=6.7cm,angle=0} \end{figure}$	Figure 2: As Fig. 1 for single events. Note that the intensity scale is not the same: contour intervals are 14 $\sigma$ and the peak is 134 $\sigma$ .
Open with DEXTER