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Table 9

Seismic data (large frequency separation Δν), masses (M) from Eq. (2), and their uncertainties (u), for a subset of Gaia FGK benchmark stars.

Name M [M] u(M) Δν [μHz] u(Δν) Ref.

Procyon 1.40 0.06 55 1 1
HD 49933 1.14 0.10 85.2 0.5 2
δ Eri 1.32 0.04 43.8 0.1 3
η Boo 1.68 0.08 39.9 0.1 4
β Hyi 1.06 0.03 57.24 0.16 5
α Cen A 1.13 0.02 106 1 6
τ Cet 0.78 0.01 169.3 0.3 7
α Cen B 0.92 0.01 161.38 0.06 8
18 Sco 1.02 0.03 134.4 0.3 9
μ Ara 0.91 0.06 90 1 10
β Vir 1.41 0.05 72.07 0.10 11
Arcturus 0.62 0.08 0.83 0.05 12
β Gem 1.96 0.09 7.14 0.12 13
ξ Hya 2.94 0.15 7.11 0.14 14

Notes. References for Δν: 1) Bedding et al. (2010), estimated from their Fig. 11; 2) Kallinger et al. (2010); 3) Bouchy & Carrier (2003); 4) Carrier et al. (2005a); 5) Bedding et al. (2007); 6) Bouchy & Carrier (2001); 7) Teixeira et al. (2009), estimated from the mean density of 2.21 ± 0.01 g cm-3 determined by the authors; 8) Kjeldsen et al. (2005), oscillations discovered by Carrier & Bourban (2003); 9) Bazot et al. (2011); 10) Bouchy et al. (2005); 11) Carrier et al. (2005b); 12) Retter et al. (2003); 13) Hatzes et al. (2012); 14) Frandsen et al. (2002), their Eq. (1).

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