Post-AGB tracks in the Hertzsprung-Russell diagram of stars at two final masses M_final = 0.55 M_⊙ and 0.58 M_⊙ for a range of metallicities. The tracks are interpolated between the data tables from Miller Bertolami (2016). The metallicity colorbar corresponds to the same coloring as found in Figs. 1 and 2. The thick lines are at the same metallicities as the ones from the original models (Z = 0.0001, 0.001, 0.01, and 0.02) and the thin lines are at Z = 0.00001, 0.0003, 0.003, 0.014, 0.05, where the middle three values are the logarithmic midpoints of the original metallicities.