Table 5: Stellar fundamental parameters from the modeling with CESAM. "s'' means at surface.
Star $\log~(L/L_{\odot})$ $T_{{\rm eff}}$ (K) Age (Myr) $M/M_{\odot}$ $R/R_{\odot}$ $\log g$ (cm s^-2) [Fe/H] $_{\rm s}$ $\overline{\Delta \nu_0}$ ( $\mu$ Hz)

$\tau$ Cet -0.296 5377 10 000 0.83 0.821 4.53 -0.31 169

$\epsilon$ Eri -0.476 5122 850 0.84 0.735 4.63 -0.06 205

$\beta$ Leo 1.165 8542 100 2.00 1.748 4.25 0.06 78

$\beta$ Pic 0.950 8073 20 1.75 1.53 4.31 -0.04 89.5

$\alpha$ PsA 1.247 8751 290 2.00 1.832 4.21 -0.10 72.8

**Table 5:** Stellar fundamental parameters from the modeling with CESAM. "s'' means at surface.
Star	$\log~(L/L_{\odot})$	$T_{{\rm eff}}$ (K)	Age (Myr)	$M/M_{\odot}$	$R/R_{\odot}$	$\log g$ (cm s^-2)	[Fe/H] $_{\rm s}$	$\overline{\Delta \nu_0}$ ( $\mu$ Hz)
$\tau$ Cet	-0.296	5377	10 000	0.83	0.821	4.53	-0.31	169
$\epsilon$ Eri	-0.476	5122	850	0.84	0.735	4.63	-0.06	205
$\beta$ Leo	1.165	8542	100	2.00	1.748	4.25	0.06	78
$\beta$ Pic	0.950	8073	20	1.75	1.53	4.31	-0.04	89.5
$\alpha$ PsA	1.247	8751	290	2.00	1.832	4.21	-0.10	72.8

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