Stellar mass function at the age of the Pleiades. Left column: lower mass clusters (M_cl(0) ≈ 1400 M_⊙); right column: more massive clusters (M_cl(0) ≈ 4400 M_⊙). The canonical IMF (Kroupa 2001) is indicated by the yellow line. Upper row: log-log MF of all stars in the cluster (solid lines) and in the tidal tail (dashed lines). Lower row: cumulative mass function for the more massive stars (m ≳ 1 M_⊙) in the tidal tail. The masses of A0, F0, and G0 star are indicated by the vertical dotted lines.