Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{0091fig1.ps} \end{figure}$ Figure 1: Top: radial velocity measurements for OGLE-TR-111, together with our orbital solution. Bottom: phase-folded normalized light curve and best-fit transit curve for OGLE-TR-111 (composed of nine partial individual transits).
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In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{0091fig2.ps} \end{figure}$ Figure 2: Left: bisector span [ $V_{\rm top} - V_{\rm bottom}$ ] for OGLE-TR-111 as a function of radial velocity. Uncertainties correspond to twice the radial velocity uncertainties. Right: phased radial velocity data with the best-fit planet orbit as a solid line. In both plots, the prediction of two blend scenarios are shown. Dotted: $M_{\rm p}=0.7~ M_\odot$ , $M_{\rm s}=0.2~ M_\odot$ , dashed: $M_{\rm p}=0.3~ M_\odot$ , $M_{\rm s}=0.2~ M_\odot$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.1cm,clip]{0091fig3.ps} \end{figure}$ Figure 3: The period-mass relation for hot Jupiters from radial velocity (triangles) and transit (stars) surveys (in the first case, minimum masses only). The large star symbol is OGLE-TR-111b. Contrarily to the three other OGLE transiting planets, OGLE-TR-111b is a "normal'' hot Jupiter in terms of mass and period.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0091fig4.ps} \end{figure}$ Figure 4: The mass-radius relation for transiting exoplanets. Jupiter and Saturn are indicated for comparison, as well as the loci of isodensities at 1.0 g cm^-3 and 0.35 g cm^-3. Data from Brown et al. 2001 (HD 290458), Konacki et al. (2003) (OGLE-TR-56), Bouchy et al. (2004a) (OGLE-TR-113), Moutou et al. (2004) (OGLE-TR-132) and this letter (OGLE-TR-111).
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{0091fig1.ps} \end{figure}$	Figure 1: Top: radial velocity measurements for OGLE-TR-111, together with our orbital solution. Bottom: phase-folded normalized light curve and best-fit transit curve for OGLE-TR-111 (composed of nine partial individual transits).
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$\begin{figure} \par\includegraphics[width=8.1cm,clip]{0091fig3.ps} \end{figure}$	Figure 3: The period-mass relation for hot Jupiters from radial velocity (triangles) and transit (stars) surveys (in the first case, minimum masses only). The large star symbol is OGLE-TR-111b. Contrarily to the three other OGLE transiting planets, OGLE-TR-111b is a "normal'' hot Jupiter in terms of mass and period.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{0091fig4.ps} \end{figure}$	Figure 4: The mass-radius relation for transiting exoplanets. Jupiter and Saturn are indicated for comparison, as well as the loci of isodensities at 1.0 g cm^-3 and 0.35 g cm^-3. Data from Brown et al. 2001 (HD 290458), Konacki et al. (2003) (OGLE-TR-56), Bouchy et al. (2004a) (OGLE-TR-113), Moutou et al. (2004) (OGLE-TR-132) and this letter (OGLE-TR-111).
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