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Table 1

Core helium burning models from Constantino et al. (2015)used in the current work.

Fig. # Colour Δ Π Our work Regularity ΔP ΔΠthis work
9 Black 240 s CHeBmodel 0 Irregular* ~241 s
9 Blue 238 s CHeBmodel 1 Irregular* ~243 s
10 Black 247 s CHeBmodel 2 Irregular
10 Blue 247 s CHeBmodel 3 Regular* ~249 s
12 Black 252 s CHeBmodel 4 Irregular* ~253 s
12 Orange 253 s CHeBmodel 5 Regular* ~253 s
12 Blue 253 s CHeBmodel 6 Regular* ~253 s
13 Blue 253 s CHeBmodel 7 Regular* ~253 s
13 Magenta 314 s CHeBmodel 8 Regular* ~316 s
14 Black 278 s CHeBmodel 9 Irregular
14 Cyan 281 sa CHeBmodel 10 Regular/spiky
16 Black 273 s CHeBmodel 11 Semi-regular* ~274 s
16 Orange 271 s CHeBmodel 12 Regular/spiky
16 Cyan 264 s CHeBmodel 13 Regular/spiky
17 Orange 268 s CHeBmodel 14 Semi-regular* ~277 s

Notes. Thefirst three columns give the figure number, the colour-code used in the figure, and the period spacing computed by Constantino et al. (2015). The last columns provide the identification that we use in this work, a comment concerning the regularity of the behaviour of the observed period spacing (Δ P) with frequency, and a rough value of our determined Δ Π for comparison purposes. The (*) indicates models for which we reliably recover Δ Π and that are used in the further analysis in this paper. (a)If the calculation includes only the region exterior to the chemical discontinuity then Δ Π = 315 s (Constantino et al. 2015).

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