\begin{table}%t1
    \caption{Stellar/planetary parameters of CoRoT-2a/b. \label{Tab:Exo2prop}}
%\centerline
 {      \begin{tabular}{l c c}
      \hline \hline
      Star$^a$  & Value $\pm$ Error & Ref.$^b$ \\
      \hline
      $P_{\rm s}$          & $(4.522 ~ \pm ~ 0.024)$ d         & L09 \\
      $P_{\rm s}^*$        & $4.57$ d                            &  \\
      Spectral type  & G7V                                 & B08 \\
      \hline  \hline
      Planet$^c$  & Value $\pm$ Error & Ref.\\\hline \\
      $P_{\rm p}$       & $(1.7429964 ~ \pm ~ 0.0000017)$ d   & A08 \\
      $T_{\rm c}$ [BJD] & $(2~454~237.53362 ~ \pm ~ 0.00014)$ d & A08 \\
      $i$            & $(87.7 ~ \pm ~ 0.2)$\textdegree & C09 \\
      $R_{\rm p}/R_{\rm s}$   & $(0.172 ~ \pm ~ 0.001)$           & C09 \\
      $a/R_{\rm s}$     & $(6.70 ~ \pm ~ 0.03)$               & A08 \\
      $u_a, u_b$      & $(0.41\pm0.03),~ (0.06\pm 0.03)$           & A08 \\
      \hline
      \end{tabular}}
\par
      \smallskip
      $^a$ {$P_{\rm s}$ -- stellar rotation period, $P_{\rm s}^*$ -- stellar rotation period used for the observation interval analyzed in this paper (see Sect.~\ref{Sec:RotPer}).}
      $^b$ {Taken from \citet{Lanza2009} [L09], \citet{Alonso2008} [A08], \citet{Bouchy2008} [B08], or \citet{Czesla2009} [C09].}
      $^c$  {$P_{\rm p}$ -- orbital period, $T_{\rm c}$ -- central time of first transit, $i$ -- orbital inclination, $R_{\rm p}, R_{\rm s}$ -- planetary and stellar radii, $a$ -- semi major axis of planetary orbit, $u_a, u_b$ -- linear and quadratic limb darkening coefficients.}\vspace*{-3mm}
\end{table}