Fig. B.1.
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Evolutionary stages of our sample. Top: Phase shift of the three central radial modes, ϵc as a function of the central large frequency separation Δνc. Bottom: period spacing ΔΠ1 as a function of Δν. The stars are colour-coded by their evolutionary stage. Orange, blue, and red circles are RGB, red clump (RC), and secondary clump (2CL), respectively. A star with ambiguous evolutionary stage is shown as a black dot. The grey-background circles correspond to the “golden sample” from CAPASS (Espinoza-Rojas et al. in prep).
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