\begin{table}%t5
\caption{\label{sum}Global parameters for the four stars. } 
%\centering
\par
\begin{tabular}{lcccccc}
\hline\hline
Star & $\nu_{\rm max}$ & $\Delta\nu$ & H$_A$/H$_B$ & $T_{\rm eff}$ & $M$ & $R$\\
 & $\mu$Hz  &  $\mu$Hz & & K & $M_{\odot}$ & $R_{\odot}$\\
\hline
102732890 & 25.5 & 3.15 & $1.1 \pm  0.1$ & 4140 & 1.2 & 13.0\\
102788308 & 51.8 & 5.3 & $1.6  \pm  0.1$ & 4260 & 1.3 & 9.4\\
102762620 & 21.9 & 2.7 & $0.3  \pm  0.03$ & 4355 & 1.5 & 15.6\\
102767771 & 25.8 & 3.1 & $0.4  \pm  0.1$ & 4250 & 1.4 & 13.7\\
\hline
\end{tabular}
\tablefoot{Frequency of maximum oscillation power ($\nu_{\rm max}$) and the large frequency separation ($\Delta\nu$) in $\mu$Hz, the ratio of the mean height of ridge ``A'' to ridge ``B'' for which the degrees are unknown, the effective temperature ($T_{\rm eff}$) in K and the asteroseismic mass and radius in~$M_{\odot}$ and $R_{\odot}$, respectively. Errors are typically of the order of~1 and 0.05~$\mu$Hz for $\nu_{\rm max}$ and $\Delta \nu$, 100~K for $T_{\rm eff}$ and below 20 and 10 \% for $M$ and $R$, respectively.}
\vspace*{4mm}
\end{table}