\begin{table}%t1
%\centering
\par
\caption{\label{tab1}The star and planet parameters from Alonso et~al. (\cite{Alonso2008}), which are used for our analysis.}
\begin{tabular}{ll}
\hline\hline
$P$~[d]      &= $1.7429964\pm0.0000017$\\
$T_{\rm c}$[d]     &= $2454237.53562\pm0.00014$\\
$T_*$ [K]    &= $5625\pm120$\\
$M_*$ [$M_{\rm{sun}}$] &=  $0.97\pm0.06$\\
$R_*$[$R_{\rm{sun}}$]  &= $0.902\pm0.018$\\
$R_{\rm p}$/$R_*$     &= $0.1667\pm0.0006$\\
$e$         &= 0 (fixed)\\
$I$ [deg]   &= $87.84\pm0.10$\\
\hline
\end{tabular}
\tablefoot{Parameter $P$ is the orbital period, $T_{\rm c}$ is the transit time, $T_*$ is the effective temperature of the star, $M_*$ and $R_*$ are the stellar mass and radius, $R_{\rm p}$/$R_*$ is the ratio of planet to star radius, $e$ is the eccentricity, and $I$ is the orbital inclination.}
\end{table}