$\begin{figure} \par\includegraphics[width=7cm,clip]{9353fig1.eps}\end{figure}$ Figure 1: Normalized and phase-folded light curve of the 34 best transits of CoRoT-Exo-1b ( top); the residuals from the best-fit model ( bottom). The bin size corresponds to 2.17 min, and the $1\sigma$ error bars have been estimated from the dispersion of the data points inside each bin.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{9353fig2.eps}\end{figure}$ Figure 2: Radial-velocity variations of CoRoT-Exo-1b versus phase from CoRoT's ephemeris. Top: the data fitted with a circular orbit of semi-amplitude $K=188~\hbox{~ms$^{-1}$ }$ and a drift of $1.02~\hbox{~ms$^{-1}$ }$ per day; bottom: the O-C residuals to the fit.
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{9353fig1.eps}\end{figure}$	Figure 1: Normalized and phase-folded light curve of the 34 best transits of CoRoT-Exo-1b ( top); the residuals from the best-fit model ( bottom). The bin size corresponds to 2.17 min, and the $1\sigma$ error bars have been estimated from the dispersion of the data points inside each bin.
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{9353fig2.eps}\end{figure}$	Figure 2: Radial-velocity variations of CoRoT-Exo-1b versus phase from CoRoT's ephemeris. Top: the data fitted with a circular orbit of semi-amplitude $K=188~\hbox{~ms$^{-1}$ }$ and a drift of $1.02~\hbox{~ms$^{-1}$ }$ per day; bottom: the O-C residuals to the fit.
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{9353fig3.eps}\end{figure}$	Figure 3: Bisector spans: no variation with amplitude and phase correlates with the radial velocities (e.g. Queloz et al. 2001).
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