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Table 1.

Stellar model settings for the different teams.

Team Birmingham Mumbai Porto
Models MESA (a) (r10398) MESA (a) (r10398) GARSTEC (b)
Oscillations GYRE GYRE ADIPLS
High-T opacities – OPAL (Iglesias & Rogers 1993, 1996) –
Low-T opacities Ferguson et al. (2005)
Gravitational settling Thoul et al. (1994)
EoS MESA/OPAL MESA/OPAL FreeEOS
Solar mixture GN93 GS98 GN93
Helium enrichment law (Y = …) 1.28855Z + 0.248 2Z + 0.24 1.1843Z + 0.2485
Nuclear reactions NACRE NACRE Solar Fusion II
Atmosphere Mosumgaard et al. (2018) Krishna Swamy (1966) Eddington
αMLT 1.037* 1.81, 1.91, 2.01 1.811
Surface correction BG14-1 BG14-1 BG14-2
Overshooting None 0 & 0.016 0.02

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