Number of meteorite-NEO pairs, N_D, with D values below a limiting threshold (red line) compared to the predicted number based on random associations (blue circles with error bars) for D_{S H} , D′, and D_H. The blue circles represent the mean number of pairs identified between 50 random samples of “meteorite falls” with the observed 35012 NEOs from 500 iterations ofKDE sampling using a bandwidth of0.15 forthe350possible50gmeteoritefalls (Fig. 5). Theblue-shaded area is within three standard deviations for random samples of 50 (the number of meteorites with orbits). The actual number of low-D value pairs correctly follows the predicted number based on random associations, indicating no evidence supporting the presence of streams in the recovered meteorite fall dataset. Two asteroids were removed as they correspond to two recovered meteorite falls, Motopi Pan and Almahata Sitta, observed telescopically before impact.