Notes. M_ini corresponds to the initial mass. N_TP, τ_{TP − (S)AGB}, and Δt_IP are, respectively, the number of thermal pulses, the duration of the TP-(S)AGB (given from the first thermal pulse until the end of our computations), and the interpulse period. M_c, ini, N_c, f and M_env, f are, respectively, the masses of the H-exhausted cores prior to the TP-(S)AGB, and the masses of the H-exhausted cores and the remnant envelopes at the end of the TP-(S)AGB. ⟨T_HeBS⟩, ⟨T_HBS⟩, ⟨T_BCE⟩ are, respectively, the temperatures at the times of maximum luminosity for each pulse, given at the centre of the He-burning shell, at the centre of the H-burning shell, and at the base of the convective envelope, and averaged over the number of thermal pulses in each sequence. is the total mass dredged-up ⟨λ⟩ was also averaged over the number of thermal pulses in each case, and ⟨Ṁ_wind⟩ is the average mass-loss rates due to winds, that is, the envelope mass lost over the duration of the (S)AGB phase. Models were calculated using both the Vassiliadis & Wood (1993) and Bloecker (1995) with η = 0.02 mass-loss rate prescription. The 6 M_⊙ model includes additional calculations with η = 0.04 and η = 1. Some of the entries for models between 4 and 7 M_⊙, computed with VW93, were presented in Tables 1 and 3 of Gil-Pons et al. (2013). We show them here to facilitate comparison.