Spatial distribution of the Pleiades cluster members having K ≤ 10 mag (from Stauffer et al. 2007), with dots proportional to the K-band brightness. The shaded area shows the path of the Moon during the time covered by our occultation events (only N-S segments through the Moon center are plotted, not its actual circular outline). The inset shows the position of the occulted sources, where cluster members are marked with squares and field stars with crosses.