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Table A.1

Stellar physical parameters obtained by the different techniques for Kepler-278 and Kepler-391.

# Method Input parameters M [M] R [R] τ [Gyr] ρ [g cm−3]
Kepler-278

1 PARAM 1.3 (Parsec iscochrones) Teff, [Fe/H], V, π 1.325 ± 0.060 2.973 ± 0.152 4.466 ± 0.630 0.071 ± 0.006
2 PARAM 1.3 (Parsec iscochrones) Teff, [Fe/H], Δν, νmax 1.227 ± 0.061 2.861 ± 0.057 5.761 ± 1.019 0.074 ± 0.005
3 q2 (Yonsei-Yale isochrones) Teff, [Fe/H], log g 1.370 ± 0.073 2.900 ± 0.241 4.200 ± 0.810 0.079 ± 0.009
4 q2 (Yonsei-Yale isochrones) Teff, [Fe/H], V, π 1.380 ± 0.150 2.850 ± 0.471 3.600 ± 1.500 0.084 ± 0.019
6 Asteroseismic scaling relations (a) Teff, Δν, νmax 1.283 ± 0.077 2.922 ± 0.058 N/A 0.072 ± 0.005
7 Direct (b) R (Fbol, Teff, π); M (R, ρ⋆,seis) 1.455 ± 0.019 3.055 ± 0.076 N/A 0.072 ± 0.002
7 Direct (b) R (Fbol, Teff, π); M (R, log g) 1.284 ± 0.384 3.055 ± 0.076 N/A 0.063 ± 0.020
8 Empirical calibration (c) Teff, [Fe/H], log g 1.274 ± 0.150 3.005 ± 0.183 N/A 0.066 ± 0.011
9 Empirical calibration (d) Teff, [Fe/H], ρ⋆,seis 1.223 ± 0.143 2.940 ± 0.095 N/A 0.068 ± 0.009

Kepler-391

1 PARAM 1.3 (Parsec iscochrones) Teff, [Fe/H], V, π 1.296 ± 0.080 2.879 ± 0.318 4.365 ± 0.899 0.077 ± 0.011
2 PARAM 1.3 (Parsec iscochrones) Teff, [Fe/H], Δν, νmax N/A N/A N/A N/A
3 q2 (Yonsei-Yale isochrones) Teff, [Fe/H], log g 1.400 ± 0.064 3.160 ± 0.189 3.700 ± 0.655 0.063 ± 0.006
4 q2 (Yonsei-Yale isochrones) Teff, [Fe/H], V, π 1.330 ± 0.134 2.580 ± 0.400 4.000 ± 1.857 0.109 ± 0.023
5 q2 (Yonsei-Yale isochrones) Teff, [Fe/H], ρ⋆,seis N/A N/A N/A N/A
6 Asteroseismic scaling relations (a) Teff, Δν, νmax N/A N/A N/A N/A
7 Direct (b) R (Fbol, Teff, π); M (R, ρ⋆,seis) N/A N/A N/A N/A
7 Direct (b) R (Fbol, Teff, π); M (R, log g) 1.461 ± 0.436 3.107 ± 0.077 N/A 0.069 ± 0.022
8 Empirical calibration (c) Teff, [Fe/H], log g 1.221 ± 0.085 2.818 ± 0.178 N/A 0.077 ± 0.009
9 Empirical calibration (d) Teff, [Fe/H], ρ⋆,seis N/A N/A N/A 0.000 ± 0.000

Notes. (a) Asteroseismic scaling relations from Kallinger et al. (2010). (b)Method detailed in Stassun et al. (2017). (c)Empirical relations of Torres et al. (2010). (d)Empirical relations of Enoch et al. (2010).

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