$\begin{figure} \par\includegraphics[width=8cm,clip]{4116fig1.eps} \end{figure}$ Figure 1: $\lambda 3968.5$ Å Ca II H absorption line region of the summed ELODIE spectra for HD 118203. No clear emission feature is observed. For clarity, spectral features due to pollution by the thorium spectrum have been removed (e.g. around $\lambda 3966.5$ Å).
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{4116fig2.eps} \end{figure}$ Figure 2: Top: last 5-months radial-velocity measurements of HD 118203 superimposed on the best Keplerian + linear drift solution indicative of a second longer-period companion in the system. Bottom: residuals around the solution. Error bars represent the photon-noise errors.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{4116fig3.eps} \end{figure}$ Figure 3: Top: phase-folded ELODIE radial-velocity measurements for the star HD 118203 after correction for the linear radial-velocity drift observed in the data. Bottom: corresponding residuals around the solution. Error bars represent the photon-noise errors.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{4116fig4.eps} \end{figure}$ Figure 4: Radial velocities (RV, upper panel) and inverse bisector slope (BIS, middle panel) phased with the orbital period P = 6.1335 d for HD 118203. The independence of the two quantities is shown by the radial velocity vs. BIS plot ( bottom panel).
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{4116fig5.eps} \end{figure}$ Figure 5: ELODIE radial velocities of HD 149143 superimposed on the derived Keplerian quasi-circular model. Residuals around the solution are displayed in the bottom panel. Error bars represent the photon-noise errors.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{4116fig6.eps} \end{figure}$ Figure 6: Phase-folded ELODIE radial velocities of HD 149143 superimposed on the derived quasi-circular Keplerian solution. Error bars represent the photon-noise errors.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{4116fig1.eps} \end{figure}$	Figure 1: $\lambda 3968.5$ Å Ca II H absorption line region of the summed ELODIE spectra for HD 118203. No clear emission feature is observed. For clarity, spectral features due to pollution by the thorium spectrum have been removed (e.g. around $\lambda 3966.5$ Å).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{4116fig2.eps} \end{figure}$	Figure 2: Top: last 5-months radial-velocity measurements of HD 118203 superimposed on the best Keplerian + linear drift solution indicative of a second longer-period companion in the system. Bottom: residuals around the solution. Error bars represent the photon-noise errors.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{4116fig3.eps} \end{figure}$	Figure 3: Top: phase-folded ELODIE radial-velocity measurements for the star HD 118203 after correction for the linear radial-velocity drift observed in the data. Bottom: corresponding residuals around the solution. Error bars represent the photon-noise errors.
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{4116fig4.eps} \end{figure}$	Figure 4: Radial velocities (RV, upper panel) and inverse bisector slope (BIS, middle panel) phased with the orbital period P = 6.1335 d for HD 118203. The independence of the two quantities is shown by the radial velocity vs. BIS plot ( bottom panel).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{4116fig5.eps} \end{figure}$	Figure 5: ELODIE radial velocities of HD 149143 superimposed on the derived Keplerian quasi-circular model. Residuals around the solution are displayed in the bottom panel. Error bars represent the photon-noise errors.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{4116fig6.eps} \end{figure}$	Figure 6: Phase-folded ELODIE radial velocities of HD 149143 superimposed on the derived quasi-circular Keplerian solution. Error bars represent the photon-noise errors.
Open with DEXTER