Table 2: Mass, age, gravity, effective temperature, luminosity, surface metallicity, acoustic depths and large separations for stellar models satisfying the observational constraints for $\iota$ Hor.
Model $M_{\star}$ ( $M_{\odot}$ ) Age (Gyr) log g log $T_{\rm eff}$ (K) log $L/L_{\odot}$ [Fe/H] $t_{\rm ac}$ (s) $\Delta \nu$ ( $\mu$ Hz)

OM1 1.140 2.231 4.38 3.786 0.207 0.11 4167 120

OM2 1.180 0.522 4.43 3.787 0.185 0.19 3876 129

AC1 1.120 2.979 4.36 3.786 0.225 0.11 4310 116

AC2 1.150 0.522 4.43 3.788 0.170 0.19 3817 131

OM3 ( $\alpha =2.2$ ) 1.190 0.508 4.46 3.797 0.191 0.26 3650 137

OM4 (Hyades) 1.180 0.627 4.42 3.790 0.202 0.14 3906 128

**Table 2:** Mass, age, gravity, effective temperature, luminosity, surface metallicity, acoustic depths and large separations for stellar models satisfying the observational constraints for $\iota$ Hor.
Model	$M_{\star}$ ( $M_{\odot}$ )	Age (Gyr)	log g	log $T_{\rm eff}$ (K)	log $L/L_{\odot}$	[Fe/H]	$t_{\rm ac}$ (s)	$\Delta \nu$ ( $\mu$ Hz)
OM1	1.140	2.231	4.38	3.786	0.207	0.11	4167	120
OM2	1.180	0.522	4.43	3.787	0.185	0.19	3876	129
AC1	1.120	2.979	4.36	3.786	0.225	0.11	4310	116
AC2	1.150	0.522	4.43	3.788	0.170	0.19	3817	131
OM3 ( $\alpha =2.2$ )	1.190	0.508	4.46	3.797	0.191	0.26	3650	137
OM4 (Hyades)	1.180	0.627	4.42	3.790	0.202	0.14	3906	128

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