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Table 1:

Mass and radius of stars used to test our asteroseismic mass and radius determination approach.
    $\nu _{\rm max}$ $\Delta \nu $ $T_{\rm eff}$   R M (R M)
    [$\mu $Hz] [K]   - - - - - - solar units - - - - - -
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)

Source LaTeX | All tables | In the text

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