\begin{table}%t1
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\par
\caption{\label{tab:params}Fitted and physical parameters found after fitting photometric and spectroscopic data of CoRoT-3b and of HD~189733b. }
\small%\centerline
{
\begin{tabular}{lll}
\hline
\hline
Parameters  (units)  & CoRoT-3b & HD~189733b \\
\hline 
\textit{Fitted parameters} &&\\ 
$D$                              &$ 0.004398 ^{\rm + 0.000084}_{- 0.000091}$         & $ 0.0200^{\rm + 0.00015}_{- 0.00017} $   \\
$K$ $({\rm m~s}^{-1})$       &$ 2169.9 ^{\rm + 35.1}_{- 22.7}$                                 & $ 201.96^{\rm + 1.07 }_{- 0.63 } $  \\
$b$ $(R_{\star})$       &$ 0.54 ^{\rm + 0.041}_{- 0.081}$                                & $ 0.6873 ^{\rm + 0.0047 }_{- 0.0078 } $ \\
$W$ (days)                 &$ 0.1566 ^{\rm + 0.0012}_{- 0.0014 }$                      & $ 0.07527^{\rm + 0.00020}_{- 0.00037} $  \\
$P$ (days)                  & $ 4.2567994 ^{\rm + 0.0000039}_{- 0.0000031}$ & $2.21857312^{\rm + 0.00000036}_{- 0.00000076} $\\
$T_0$ (bjd)                 &$ 54283.13388 ^{\rm + 0.00026}_{- 0.00022}$         &$53988.80339^{\rm + 0.000072}_{- 0.000039} $\\
$e~\cos(\omega_0)$  &$ -0.0083 ^{\rm + 0.0054}_{- 0.0041}$                     & $0.0038^{\rm +0.0020}_{-0.0020}$\\
$e~\sin(\omega_0)$   &$ 0.000 ^{\rm + 0.021}_{- 0.020}$                             & $-0.0017^{\rm +0.0024}_{-0.0034}$\\
$V~\sin(I)~\cos(\beta)$ &$ 28.4 ^{\rm + 6.5}_{- 5.6}$                                        & $3.316^{\rm +0.017}_{-0.068}$ \\
$V~\sin(I)~\sin(\beta)$  &$ 21.9 ^{\rm + 8.3}_{- 14.1}$                                      & $0.049^{\rm +0.018}_{-0.017}$ \\
$\Gamma$ $({\rm m~s}^{-1}~{\rm yr}^{-1})$           & --                                                   &  $ -0.2 ^{\rm + 2.7}_{- 3.9}$\\ 
&&\\
\textit{Derived parameters}       &      &  \\ 
&&\\
$R_{\rm p} / R_{\star}$                         & $ 0.06632 ^{\rm + 0.00063}_{- 0.00069} $  & $ 0.15812 ^{\rm + 0.00046}_{- 0.00052}$ \\
& & \\
$R_{\star} / a$                               & $ 0.1257^{\rm + 0.0057 }_{- 0.0064} $  & $ 0.1142 ^{\rm + 0.0006}_{- 0.0012} $\\
$\rho_{\star}$   $(\rho_{\odot})$ & $ 0.372^{\rm + 0.064 }_{- 0.047} $         &$ 1.831 ^{\rm + 0.059}_{- 0.029}$  \\
$R_{\star}$  $(R_{\odot})$          & $1.540^{0.083}_{0.078}$                  & $ 0.766 ^{\rm + 0.007}_{- 0.013}  $\\
$M_{\star} $  $(M_{\odot})$        & $ 1.359^{\rm + 0.059 }_{- 0.043}$          & $ 0.823 ^{\rm + 0.022}_{- 0.029} $\\
$V~\sin(I)$ $({\rm km~s}^{-1})$              &$ 35.8 ^{\rm + 8.2}_{- 8.3}$                      &$ 3.316 ^{\rm + 0.017}_{- 0.067}$ \\
& & \\
$R_{\rm p} / a$                               & $ 0.00834^{\rm + 0.00042 }_{- 0.00050} $  & $ 0.01805 ^{\rm + 0.00011}_{- 0.00025} $\\
$R_{\rm p}$  $(R_J)$                    & $ 0.9934^{\rm + 0.058}_{- 0.058} $              & $ 1.178 ^{\rm + 0.016}_{- 0.023} $\\
$M_{\rm p}$ $(M_J)$                    & $21.23 ^{\rm + 0.82}_{- 0.59}$                       & $ 1.138 ^{\rm + 0.022}_{- 0.025} $\\
&&     \\
$a$ (AU)                        & $ 0.05694 ^{\rm + 0.00096}_{- 0.00079} $      &$ 0.03120 ^{\rm + 0.00027}_{- 0.00037} $\\
$i$   $(^{\circ})$                 & $ 86.10 ^{\rm + 0.73}_{- 0.52} $                        & $ 85.508 ^{\rm + 0.10}_{- 0.05} $\\
$e$                                      & $  0.008 ^{\rm + 0.015}_{- 0.005} $                   & $ 0.0041 ^{\rm + 0.0025}_{- 0.0020} $\\
$\omega_0$  $(^{\circ})$ & $179 ^{\rm + 170}_{- 170}$                               &  $ -24.1 ^{\rm + 33.9}_{- 34.5}$\\
$\beta$ $(^{\circ})$           & $37.6^{\rm +10.0}_{-22.3}$                               &  $ 0.85 _{- 0.32}^{\rm + 0.28}$\\ 
$\gamma$ \textit{Velocities} (${\rm m~s}^{-1}$)\\
\\
\textit{Sophie}&--56182.46& --2273.59\\
\textit{TLS}&--56652.08&\\
\textit{Keck}&--&--15.84\\
\textit{Harps}&--56156.08&--2161.14\\
\textit{Harps} (RM)&--56160.84&--2191.92\\
&--&--2225.44\\
&--&--2204.07\\
\\
\textit{Normalisation factors}\\
\\
\textit{CoRoT} & 0.9999998&--\\
\textit{FLWO 1.2~m $z$-band} &--&0.99974 \\
\textit{T10 ($b+y$)/2 band} &--&0.99977 \\
\textit{MAGNUM 2~m $V$-band} &--&0.99979 \\
\textit{Wise 1~m $I$-band} &--&0.99977 \\
\\
$\chi^2_{\rm reduced}$           & $1.17\pm0.08$ &  $ 1.21\pm 0.03$\\
&&\\
\hline
\end{tabular}}
\smallskip
The reduced $\chi^2$ were calculated with 414 degrees of freedom for CoRoT-3b and 2890 for HD~189773b.\\  {Nota Bene}: $\beta = -\lambda$; $\beta$ is used since the first reference of a projected spin-orbit angle was named thus, in \citet{Hosokawa:1953p2002}. $V~\sin(I)$s are probably overestimated, see Sect.~\ref{sec:res} for details.
\end{table}