Binned distributions M_j of semimajor axes a and inclinations i of synthetic NEO orbits, originating from individual asteroid families. The colors correspond to the number of test particles in bins, although the quantity M_j(a, i) was eventually normalized. The bin sizes were 0.01 au and 1°, respectively. The Apophis orbit is marked with a black cross. The orbits of other LL-like NEOs from Binzel et al. (2019); Marsset et al. (2022) are marked with gray crosses. Of the three, the highest density for producing Apophis-like objects is from the Flora family.