Relevant TP-(S)AGB parameters for intermediate-mass models of different metallicities calculated with similar versions of the Monash-Mount Stromlo stellar evolution code. M_core is the core mass at the end of the TP-(S)AGB calculations, λ is the average TDU parameter, τ_TPAGB is the duration of the TP-(S)AGB phase, T_BCE is the maximum temperature at the base of the convective envelope, N_TP is the number of thermal pulses, t_IP is the average interpulse period, L_MAX is the maximum luminosity, and Ṁ is the average mass-loss rate during the TP-(S)AGB phase. Values are shown for our Z = 10⁻⁵ models (black); for Z = 10⁻⁴ models from Karakas (2010; dotted orange), and from Doherty et al. (2014b, 2015; solid orange); for Z = 10⁻³ models for Fishlock et al. (2014; thin green) and Doherty et al. (2014b, 2015; thick green). Sequences calculated with the wind prescriptions by VW93, Reimers (1975), and Blo95 are shown, respectively, with solid, dotted and dashed lines.