$\begin{figure} \par\includegraphics[width=7.5cm,clip]{6029fig1.ps} \end{figure}$ Figure 1: The CaII K absorption line of the ELODIE spectrum of HD 185269, which shows no emission feature in its core.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{6029fig2.eps}\end{figure}$ Figure 2: The inverse slope of the bisector is shown against the radial-velocity measurements of HD 185269. No correlation is observed.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{6029fig3.eps} \end{figure}$ Figure 3: Radial-velocity measurements of HD 185269 superimposed on the best Keplerian solution. Error bars represent the photon-noise uncertainties.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{6029fig4.eps} \end{figure}$ Figure 4: Phase-folded radial velocity measurements of HD 185269 superimposed on the best Keplerian solution. Error bars represent the photon-noise uncertainties. Bottom plot: residuals as a function of time.
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{6029fig1.ps} \end{figure}$	Figure 1: The CaII K absorption line of the ELODIE spectrum of HD 185269, which shows no emission feature in its core.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{6029fig2.eps}\end{figure}$	Figure 2: The inverse slope of the bisector is shown against the radial-velocity measurements of HD 185269. No correlation is observed.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{6029fig3.eps} \end{figure}$	Figure 3: Radial-velocity measurements of HD 185269 superimposed on the best Keplerian solution. Error bars represent the photon-noise uncertainties.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{6029fig4.eps} \end{figure}$	Figure 4: Phase-folded radial velocity measurements of HD 185269 superimposed on the best Keplerian solution. Error bars represent the photon-noise uncertainties. Bottom plot: residuals as a function of time.
Open with DEXTER