\begin{table}%t1 %\centering \par \caption{\label{table_parameters}Parameters for the \cible\ system.} \begin{tabular}{lcc} \hline \hline Parameters & Values and 1-$\sigma$ error bars & Unit \\ \hline \multicolumn{3}{l}{{\hspace{-0.25cm}}Free parameters constrained by photometry only} \\ $R_{\rm p}/R_*$ & $0.1001 \pm 0.0006$ \\ $a/R_*$ & $97.0 \pm 1.6$ \\ \hline \multicolumn{3}{l}{{\hspace{-0.25cm}}Free parameters constrained both by photometry and radial velocities} \\ $a \cos i /R_*$ & $1.238 \pm 0.011$ \\ $P$ & $111.4367 \pm 0.0004$ & days \\ $T_0$ (periastron) & $2~455~204.916 \pm 0.004$ & HJD \\ $e \cos \omega$ & $ 0.4774 \pm 0.0018$ \\ $e \sin \omega$ & $-0.8016 \pm 0.0017$ \\ $K \sqrt{1-e^2}$ & $171.1 \pm 0.5$ & \ms \\ \hline \multicolumn{3}{l}{{\hspace{-0.25cm}}Free parameters constrained by radial velocities only} \\ $V_{\textrm{ELODIE}}$ & $3.7888\pm 0.0023$ & \kms \\ \hspace{0.5cm} $\sigma$(O--C) & 17.8 & \ms \\ $V_{\textrm{HRS}}$ & $-0.0193 \pm 0.0019$ & \kms \\ \hspace{0.5cm} $\sigma$(O--C) & 6.3 & \ms \\ $V_{\textrm{HIRES}{\rm ,~pre-ugrade}}$ & $-0.1845 \pm 0.0010$ & \kms \\ \hspace{0.5cm} $\sigma$(O--C) & 5.5 & \ms \\ $V_{\textrm{HIRES}{\rm ,~post-ugrade}}$ & $-0.1827 \pm 0.0007$ & \kms \\ \hspace{0.5cm} $\sigma$(O--C) & 2.4 & \ms \\ \hline \multicolumn{3}{l}{{\hspace{-0.25cm}}Directly derived parameters} \\ $b$ & $0.808 \pm 0.007$ \\ $i$ & $89.269 \pm 0.018$ & $^{\circ}$\\ $T_{\rm t}$ (transit mid-time) & $2~455~210.6420 \pm 0.0010$ & HJD \\ Transit duration $T_{1-4}$ & $11.88 \pm 0.09$ & h \\ Transit duration $T_{1-2} =T_{3-4}$ & $2.78 \pm 0.10$ & h \\ $e$ & $0.9330 \pm 0.0005$ \\ $\omega$ & $300.77 \pm 0.15$ & $^{\circ}$ \\ $K$ & $475.3 \pm 2.0$ & \ms \\ $\rho_*$ & $1.39 \pm 0.07$ & g/cm$^3$\\ \hline $T_{\rm e}$ (eclipse mid-time) & $2~454~424.736 \pm 0.003$\tablefootmark{\ddag} & HJD \\ Eclipse duration $T_{1-4}$ & $1.85 \pm 0.14$\tablefootmark{\ddag} & h \\ \hline \multicolumn{3}{l}{{\hspace{-0.25cm}}Derived parameters assuming a $M_\star$-value} \\ $M_\star$ & $1.01 \pm 0.05$\tablefootmark{\dagger} & $M_\odot$ \\ $R_\star$ & $1.007 \pm 0.024$ & $R_\odot$ \\ $M_\textrm{p}$ & $4.08 \pm 0.14$ & $M_{\rm Jup}$\\ $R_\textrm{p}$ & $0.981 \pm 0.023$ & $ R_{\rm Jup}$ \\ $\rho_{_\textrm{p}}$ & $5.4 \pm 0.4$ & g/cm$^3$\\ $a$ & $0.455 \pm 0.008 $ & AU \\ \hline \multicolumn{3}{l}{{\hspace{-0.25cm}}Rossiter-McLaughlin effect} \\ $V \sin I_*$ & $1.7 \pm 0.3$ & \kms \\ $\lambda$ & $42 \pm 8$ & $^{\circ}$\\ $V_{\textrm{SOPHIE}{\rm ,~transit~February~09}}$ & $3.9162 \pm 0.0013$ & \kms \\ \hspace{0.5cm} $\sigma$(O--C) & 4.3 & \ms \\ $V_{\textrm{HIRES}{\rm ,~post-ugrade,~transit~June~09}}$ & $-0.1795 \pm 0.0011$ & \kms \\ \hspace{0.5cm} $\sigma$(O--C) & 0.7 & \ms \\ $V_{\textrm{SOPHIE}{\rm ,~transit~January~10}}$ & $3.9018 \pm 0.0013$ & \kms \\ \hspace{0.5cm} $\sigma$(O--C) & 5.2 & \ms \\ \hline \end{tabular} \tablefoot{ \tablefoottext{\dagger}{Combined value from Pont et~al. (\cite{pont09}) and Winn et~al. (\cite{winn09a});} \tablefoottext{\ddag}{from Laughlin et~al. (\cite{laughlin09}).} }\vspace*{2mm} \end{table}