Notes. For each asteroid, the table gives the ecliptic coordinates λ₁ and β₁ of the pole solution with the lowest χ², the corresponding mirror solution λ₂ and β₂, the sidereal rotational period P, the number of dense lightcurves N_lc observed during N_app apparitions, and the number of sparse data points for the corresponding observatory: N₆₈₉, N₇₀₃, and N₉₅₀. The uncertainty of the sidereal rotational period corresponds to the last decimal place of P and of the pole direction to 5–10° if we have multi-apparition dense data or 10–20° if the model is based mainly on sparse data (i.e., only a few dense lightcurves from 1–2 apparitions).