Fit of the oscillation pattern of the evolved RGB star KIC 2443903, near the limit of capability of identification, with a large crowding due to the high mode density. The second rotation crossing, where all m components apparently coincide, occurs at n = −189 (with an abscissa ≃0.1 and n_p = 9); the third crossing, where |m| = 1 components apparently coincide with m = 0 inbetween, occurs at n = −233 (with an abscissa ≃0.25 and n_p = 7). Same style as Fig. 2. Note that the modes with large heights at an abscissa ≃ 0.2 are ℓ = 3 modes.