Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=8.8cm,height=5cm,clip]{Ff111_f2.eps} \end{figure}$ Figure 2: Rate induced by galactic 511 keV photons as a function of longitude. The response to a Gaussian source ( $FWHM = 10\ensuremath {^\circ }$ ) is also shown for comparison.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,height=5.0cm,clip]{Ff111_f3.eps} \end{figure}$ Figure 3: 511 keV flux spectrum obtained using a Gaussian centred on the GC with a FWHM of 10 $\ensuremath {^\circ }$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,height=5.0cm,clip]{Ff111_f1.eps} \end{figure}$	Figure 1: Raw spectrum and background model components.
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$\begin{figure} \par\includegraphics[width=8.8cm,height=5cm,clip]{Ff111_f2.eps} \end{figure}$	Figure 2: Rate induced by galactic 511 keV photons as a function of longitude. The response to a Gaussian source ( $FWHM = 10\ensuremath {^\circ }$ ) is also shown for comparison.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,height=5.0cm,clip]{Ff111_f3.eps} \end{figure}$	Figure 3: 511 keV flux spectrum obtained using a Gaussian centred on the GC with a FWHM of 10 $\ensuremath {^\circ }$ .
Open with DEXTER