Top: number counts as a function of the radius of GCs (in yellow), PNe (in green), and the total population (in gray). The overdensity of PNe around NGC 1387 is clearly seen at R ∼ 20″ (see text). Bottom: radial density distribution of GCs (yellow open dots), PNe (green), and the total population (black), arbitrarily re-scaled to match the surface brightness of the Fornax core from I+16 (gray tick line). Error bars represent Poissonian errors on the tracer counts.