$\begin{figure} \par\includegraphics[width=16.2cm,clip]{f1_9277.ps} \end{figure}$ Figure 1: The Swift/BAT light curve of A0535+26 during the normal outburst in August/September 2005. The smooth solid line shows the pulse period development as measured by RXTE (from Caballero et al. 2007b). The dashed line shows the time of periastron passage.
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In the text

$\begin{figure} \par\includegraphics[width=16.2cm,clip]{f1_9277.ps} \end{figure}$	Figure 1: The Swift/BAT light curve of A0535+26 during the normal outburst in August/September 2005. The smooth solid line shows the pulse period development as measured by RXTE (from Caballero et al. 2007b). The dashed line shows the time of periastron passage.
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