Fig. B.1.
Fit of the oscillation pattern of the RGB star KIC 5024476, member of the open cluster NGC 6819. The dim magnitude of the cluster stars explains the low S/N. However, unambiguous doublets are identified all along the mixed-mode spectrum; m = 0 modes are mostly absent and |m| = 1 modes dominate the mixed-mode spectrum, so that a nearly pole-on inclination is not possible. Same style as Fig. 2.
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