\begin{table}%t3
%\centering
\par
\caption {\label{tab:fits_btfr}Results of the linear fits 
to the high-mass end ($M_{*} >  10^9  ~{M_{\odot}}~ h^{-1}$) of the bTFR 
for S230 at $z=0$.}
{
\begin{tabular}{lcc}\hline \hline
\noalign{\smallskip}
$V_{\rm i}$ & $Y_{100}$  &  $\alpha$ \\  \hline
 $V_{\rm circ}$ at $0.5 R_{\rm bar}$  & $9.64 \pm 0.20$    & $3.19 \pm 0.07$    \\
 $V_{\rm circ}$ at $R_{\rm bar}$      & $9.56 \pm 0.23$    & $3.23 \pm 0.08$    \\
 $V_{\rm circ}$ at $1.5 R_{\rm bar}$  & $9.57 \pm 0.25$    & $3.14 \pm 0.08$    \\
 $V_{\rm max}$                        & $9.55 \pm 0.24$    & $3.22 \pm 0.08$ \\ 
\hline 
\end{tabular}
}
\tablefoot {
Column 1: Kinematic indicator used for the calculations.
Column 2: Baryonic mass corresponding to a velocity of $100~ {\rm  km ~ s}^{-1}$  according to the fitting. 
Column 3: Slope derived from the linear \mbox{regression}.}
\end{table}