\begin{table}%t1 \caption{\label{tab:Tstars}Mass and radius of stars used to test our asteroseismic mass and radius determination approach.} %\centering \small \begin{tabular}{lccccccclr} \hline \hline\noalign{\smallskip} &&$\nu_{\rm max}$&$\Delta \nu$&$T_{\rm eff}$&&$R$ &$M$ & ($R$ & $M$)\\ &&\multicolumn{2}{c}{[$\mu$Hz]}&[K]&&\multicolumn{4}{c}{- - - - - - solar units - - - - - -}\\ \hline Arcturus &&3.47 $\pm$ 0.03 &0.825 $\pm$ 0.05 &4290 $\pm$ 30 &&27.9 $\pm$ 3.4 &0.8 $\pm$ 0.2&(25.4 $\pm$ 0.3 &0.7--2.0)\\ HD181907 &&29.1 $\pm$ 0.6 &3.47 $\pm$ 0.12 &4760 $\pm$ 65 &&13.1 $\pm$ 1.0 &1.5 $\pm$ 0.23&(12.3 $\pm$ 0.6 &1.5--2.0)\\ $\beta$ Oph &&46.0 $\pm$ 2.5 &4.1 $\pm$ 0.2 &4470 $\pm$ 100 &&14.9 $\pm$ 1.7 &3.1 $\pm$ 0.8 &(12.2 $\pm$ 0.8 &$\leq$3.2)\\ $\epsilon$ Oph &&53.5 $\pm$ 2 &5.2 $\pm$ 0.1 &4877 $\pm$ 100 &&10.7 $\pm$ 0.6 &1.8 $\pm$ 0.3&(10.4 $\pm$ 0.5 &2.02)\\ $\xi$ Hya &&92.3 $\pm$ 3 &7.0$\pm0.2$ &5010 $\pm$ 50 &&10.2 $\pm$ 0.7 &2.9 $\pm$ 0.4&(10.4 $\pm$ 0.5 &2.93--3.15)\\ M~67 13 &&208.9 $\pm$ 4 &15.9 $\pm$ 0.2 &4966 $\pm$ 50 &&4.6 $\pm$ 0.1 &1.33 $\pm$ 0.1&(4.3 $\pm$ 0.3 &1.35)\\ $\nu$ Ind &&313 $\pm$ 10 &24.25 $\pm$ 0.25 &5300 $\pm$ 100 &&3.04 $\pm$ 0.12 &0.91 $\pm$ 0.1&(2.96 $\pm$ 0.13 &0.81--0.89)\\ $\zeta$ Her A &&700 $\pm$ 50 &43 $\pm$ 0.5 &5825 $\pm$ 50 &&2.3 $\pm$ 0.17 &1.2 $\pm$ 0.26&(2.51 $\pm$ 0.11 &1.3--1.5)\\ $\beta$ Hyi &&1020 $\pm$ 50 &56.2 $\pm$ 0.2 &5872 $\pm$ 44 &&1.94 $\pm$ 0.1 &1.28 $\pm$ 0.2&(1.81 $\pm$ 0.02 &1.0--1.2)\\ HD49933 &&1657 $\pm$ 28 &85.2 $\pm$ 0.5 &6500 $\pm$ 75 &&1.44 $\pm$ 0.03 &1.21 $\pm$ 0.07&(1.46 $\pm$ 0.05 &1.325)\\ $\mu$ Ara &&1900 $\pm$ 50 &90 $\pm$ 1 &5813 $\pm$ 40 &&1.40 $\pm$ 0.05 &1.23 $\pm$ 0.1&(1.36 $\pm$ 0.03 &1.1--1.3)\\ $\alpha$ Cen A&&2410 $\pm$ 130 &106 $\pm$ 0.2 &5770 $\pm$ 50 &&1.28 $\pm$ 0.07 &1.30 $\pm$ 0.2&(1.26 $\pm$ 0.03 &1.124 $\pm$ 0.008)\\ $\alpha$ Cen B&&4090 $\pm$ 170 &161.4 $\pm$ 0.06 &5300 $\pm$ 50 &&0.90 $\pm$ 0.04 &1.04 $\pm$ 0.13&(0.85 $\pm$ 0.02 &0.934 $\pm$ 0.007)\\ \hline \end{tabular} \vspace*{3mm} \end{table}