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Table 3

Characteristics of each model set used for inferring the stellar parameters of the two stars.

Characteristics Verma Lebreton Ball Creevey

Evolution code MESA1 CESAM2K2 MESA1 ASTEC3
Oscillation code ADIPLS4 LOSC 5 ADIPLS 4 ADIPLS4
Opacities OP OPAL96/Wichita OPAL96 OPAL96
EOS OPAL05 OPAL05 OPAL05 OPAL05
Nuclear reaction rates NACRE6+LUNA7 NACRE6 + LUNA7 NACRE6 NACRE6
Atomic diffusion TBL94 MP93 TBL94 MP93
Convection CG68 CGM96 H65 BV58
Overshoot H00 M75 H00 M75
corr GS98 GN93 GS98 GN93
Boundary conditions Grey Eddington atm. Grey Eddington atm. Grey Eddington atm. Grey Eddington atm.
Grid model parameters M, [Fe/H], Yi, αCONV, αOV M, Age, Yi, Zi, αCONV,αOV,A
Free model parameters M,Age,Yi, [ Fe / H ] ,αCONV,αOV M,Age,Yi, [ Fe / H ] ,αCONV,αOV
Frequency surface correction KBC08 KBC08 BG14 None
Optimisation ⟨ Δν, δν, r01, r02, [Fe/H] ν, Teff, [Fe/H], L ν, Teff, [Fe/H], L r01, r02, Δν0, LB/LA, lowest ν(l = 0)
Regularisation L, Teff/M, R No No No

Notes. 1) Modules for Experiments in Stellar Astrophysics (Paxton et al. 2011, 2013). 2) Code d’Evolution Stellaire Adaptatif et Modulaire (Morel & Lebreton 2008; Marques et al. 2013). 3) The Aarhus STellar Evolution Code (Christensen-Dalsgaard 2008b). 4) The Aarhus adiabatic oscillation package (Christensen-Dalsgaard 2008a). 5) Liège OScillation Code: (Scuflaire et al. 2008). 6) Nuclear Astrophysics Compilation of REaction rates (Angulo et al. 1999). 7) Laboratory Underground Nuclear Astrophysics (Formicola et al. 2004). OP: Badnell et al. (2005), Seaton (2005); Wichita: Ferguson et al. (2005); OPAL96: Iglesias & Rogers (1996). OPAL05: Rogers & Nayfonov (2002). TBL94: Thoul et al. (1994); MP93: Michaud & Proffitt (1993). CG68: Cox & Giuli (1968); BV58: Böhm-Vitense (1958); CGM96: Canuto et al. (1996); H65: Henyey et al. (1965). M75: Maeder (1975); H00: Herwig (2000). GN93: Grevesse & Noels (1993); GS98: Grevesse & Sauval (1998). KBC08: Kjeldsen et al. (2008); BG14: Ball & Gizon (2014).

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