Detection of rotation and of octupole modes in the MS star KIC 12069424 (left panels) and in the late SG star KIC 4351319 (right panels) using a scheme similar to Fig. 8. Top panels: a close-up to the chunk ℓ = 1 rotational triplet and its adjacent ℓ = 3 for the MS star, and to the ℓ = 1 rotational triplets of two mixed modes of the same chunk for the late SG star, with the ℓ = 3 mode included. The mode identification (n,ℓ,m) as obtained by FAMED is indicated. The orange downward arrows mark the asymptotic position of the ℓ = 3 modes. Middle and bottom panels: ASEF showing ν_f, i, σ_f, i, r_a, b, before and after the peak rotation tests.