Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Gb021_f3.eps}\end{figure}$ Figure 3: Spin-pulse profiles of XTE J1807-289 at different orbit phases in the energy range 0.5-10 keV. In dotted red the orbit averaged folded spin light curve from Fig. 2 in the same energy range.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Gb021_f4.eps}\end{figure}$ Figure 4: Pulsed fraction values for 6 orbital phases indicated by different symbols for all the four orbits in the 0.5-3.0 keV energy band.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Gb021_f1.eps}\end{figure}$	Figure 1: $\chi ^{ 2}$ grid search of the orbital parameters. See text for details.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Gb021_f2.eps}\end{figure}$	Figure 2: Spin-pulse profiles of XTE J1807-289 in different energy bands.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Gb021_f3.eps}\end{figure}$	Figure 3: Spin-pulse profiles of XTE J1807-289 at different orbit phases in the energy range 0.5-10 keV. In dotted red the orbit averaged folded spin light curve from Fig. 2 in the same energy range.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Gb021_f4.eps}\end{figure}$	Figure 4: Pulsed fraction values for 6 orbital phases indicated by different symbols for all the four orbits in the 0.5-3.0 keV energy band.
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