\begin{table}%t6
\caption{\label{table_stel_parm}Stellar parameters for~CoRoT-6 derived through modeling spectra and using the 4~methods described in the text. The errors are 1$\sigma$.}
%\centering
  \begin{tabular}{llllllll}
\hline \hline \noalign{\smallskip}
Method & \teff & $\log~g$& [Fe/H] & $V_{\rm micro}$ & $V_{\rm macro}$ & $v~{\rm sin}~i$ & Comment\\
 & K &&& (km~s$^{-1}$) & (km~s$^{-1}$) &(km~s$^{-1}$) &\\
\hline
1. (SME 2.1) & $6090 \pm 70$ & $4.43 \pm 0.1$ & $-0.20 \pm 0.1$ & $1.2 \pm 0.10$ & $3.5 \pm 1.0$ & $7.6 \pm 1.0$ & $\log~g$ determined from fitting \\
& & & & & & & the line wings of Mg~I, Ca~I and Na~I \\
2. (VWA) &  $6090 \pm 50$ & $4.37 \pm 0.062$ & $-0.20 \pm 0.08$ & $1.24 \pm 0.10$ & $3.0 \pm 1.0$ & $8.0 \pm 1.0$ & \\
3.  & $6050 \pm 100$ & $4.05 \pm 0.2$  & $-0.18 \pm 0.15$ & -- & -- & $7.0 \pm 1.0$ & \\
4. & $6006 \pm 73$ & -- & -- & -- & -- & -- & \\
5. & $F9$\tablefootmark{\dagger} & $V$\tablefootmark{\ddagger} & $-0.40$ to $-0.10$ & -- & -- & -- & Fitting of low \\
& & & & & & & dispersion spectra \\
\hline
\end{tabular}
\tablefoot{\tablefoottext{\dagger}{Spectral type from template fitting.} \tablefoottext{\ddagger}{Luminosity class from template fitting}.}
\end{table}