$\begin{figure} \par\includegraphics[width=9cm,clip]{9498im.eps}\end{figure}$ Figure 1: CCD frame observed at 23/08/2003, $\rm 4^h 7^m 27^s$ UTC. Exposure time $\rm 1^s$ . CCD dimension 1050 $\times$ 1050 square pixels.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{9498his.eps}\end{figure}$ Figure 2: Histogram for the right ascension and declinations residuals, in arcseconds, of Martian satellites. The $\rm (O{-}C)\alpha$ and $\rm (O{-}C)\delta$ are $(\alpha _{\rm observed}-\alpha _{\rm calculated})$ and $(\delta _{\rm observed}-\delta _{\rm calculated})$ , respectively.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{9498rpho.eps}\end{figure}$ Figure 3: Residuals $({\rm O{-}C})_{\alpha ,\delta }$ , in arcseconds, for the Phobos satellite as a function of time.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{9498rdei.eps}\end{figure}$ Figure 4: Residuals $({\rm O{-}C})_{\alpha ,\delta }$ , in arcseconds, for the Deimos satellite as a function of time.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{9498im.eps}\end{figure}$	Figure 1: CCD frame observed at 23/08/2003, $\rm 4^h 7^m 27^s$ UTC. Exposure time $\rm 1^s$ . CCD dimension 1050 $\times$ 1050 square pixels.
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$\begin{figure} \par\includegraphics[width=9cm,clip]{9498his.eps}\end{figure}$	Figure 2: Histogram for the right ascension and declinations residuals, in arcseconds, of Martian satellites. The $\rm (O{-}C)\alpha$ and $\rm (O{-}C)\delta$ are $(\alpha _{\rm observed}-\alpha _{\rm calculated})$ and $(\delta _{\rm observed}-\delta _{\rm calculated})$ , respectively.
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$\begin{figure} \par\includegraphics[width=9cm,clip]{9498rpho.eps}\end{figure}$	Figure 3: Residuals $({\rm O{-}C})_{\alpha ,\delta }$ , in arcseconds, for the Phobos satellite as a function of time.
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$\begin{figure} \par\includegraphics[width=9cm,clip]{9498rdei.eps}\end{figure}$	Figure 4: Residuals $({\rm O{-}C})_{\alpha ,\delta }$ , in arcseconds, for the Deimos satellite as a function of time.
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