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Table 1.

Seismic and spectroscopic parameters of the six seismic solar analogs.

Identifier A2Z Universal pattern with apollinaire Spectroscopic parameters

νmax Δν νmax Δν ϵ nfit Teff log g [Fe/H] v sin i
[μHz] [μHz] [μHz] [μHz] [–] [–] [K] [dex] [dex] [km/s]
EPIC 206064678 (a) 3272 ± 93 138.06 ± 3.97 3146 ± 118 137.80 ± 0.18 1.564 ± 0.029 5 5476 ± 55 4.41 ± 0.11 0.25 ± 0.07 2.3 2.1 + 1.5 Mathematical equation: $ ^{+1.5}_{-2.1} $
EPIC 206245055 (b) 3187 ± 76 138.69 ± 3.71 3129 ± 52 138.78 ± 0.18 1.485 ± 0.029 5 5841 ± 54 4.47 ± 0.17 −0.39 ± 0.09 3.3 2.1 + 1.5 Mathematical equation: $ ^{+1.5}_{-2.1} $
EPIC 206371648 (c) 2972 ± 70 139.03 ± 4.82 2993 ± 63 136.02 ± 0.18 1.512 ± 0.026 9 5573 ± 43 4.37 ± 0.17 −0.26 ± 0.06 4.7 2.0 + 1.4 Mathematical equation: $ ^{+1.4}_{-2.0} $
EPIC 212624487 (d) 3109 ± 150 130.78 ± 3.70 3072 ± 21 132.75 ± 0.10 1.387 ± 0.017 9 6038 ± 27 4.50 ± 0.15 −0.16 ± 0.09 4.7 2.5 + 1.8 Mathematical equation: $ ^{+1.8}_{-2.5} $
EPIC 212708252 (e) 2930 ± 84 135.11 ± 4.09 2913 ± 20 133.40 ± 0.05 1.542 ± 0.008 9 5579 ± 43 4.42 ± 0.13 −0.09 ± 0.07 2.2 2.1 + 1.5 Mathematical equation: $ ^{+1.5}_{-2.1} $
KIC 3241581 (f) 2751 ± 122 122.90 ± 1.60 2828 ± 171 122.84 ± 0.88 1.435 ± 0.276 5 5730 ± 50 4.39 ± 0.13 0.25 ± 0.06 3.5 2.2 + 1.6 Mathematical equation: $ ^{+1.6}_{-2.2} $

Notes. The star’s identifier is the Ecliptic Plane Input Catalog (EPIC; Huber et al. 2016) or the Kepler Input Catalog (KIC; Brown et al. 2011). The frequency of maximum power, νmax, and large separation, Δν, are given from the A2Z pipeline. The Universal pattern parameters computed with the apollinaire code include νmax; Δν; the phase offset, ϵ; and the number of fitted radial orders, nfit. Spectroscopic parameters include effective temperature, Teff; surface gravity, log g; metallicity, [Fe/H]; and projected rotational velocity, v sin i, all with their respective uncertainties.

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