Asteroseismology of the young open cluster NGC 2516 - II. Constraining cluster age using gravity-mode pulsators

Open Access

Fig. C.1.

Same as Fig. 2 for TIC 308307454, but using Approach 2. The bottom-right panel shows the distributions of the joint age derived using Approach 2, so this panel is identical in Figs. C.3, C.5, and C.7.

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