Fit of the oscillation pattern of the RGB star KIC 2437976, member of the open cluster NGC 6791. The dim magnitude of the cluster stars explains the low S/N. The identification at radial order 9, supported by the radial orders 8 and 10, is unambiguously conclusive: m = 0 modes are mostly absent and |m| = 1 modes dominate the mixed-mode spectrum, so that a pole-on inclination is not possible. Same style as Fig. 2.