Proper element catalogs and asteroid families

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Dynamical erosion of the asteroid belt and implications for large impacts in the inner Solar System (2009, methodology): “The observational data set we used was the 1137 asteroids with H 6 10:8 obtained from the AstDys online data service (Knežević and Milani, 2003).”
Yarkovsky/YORP chronology of asteroid families (2006, methodology): “The main obstacle here is obtaining a large enough sample of asteroid proper elements (e.g., Knežević and Milani, 2000, 2003; Knežević et al., 2002) to compute when the fragments all shared the same approximate starting orbit (note young families are statistically expected to be in the same time…”
The primordial excitation and clearing of the asteroid belt—Revisited (2006, methodology): “…and Saturn on the orbits predicted by the Nice Model (the CJS simulations), compared to the actual proper elements of asteroids larger that ∼50 km (Kneževi´c and Milani, 2003). the depletion due to the embedded planetary embryos described above, is sufficient to explain the current mass of the…”
Strong chaos induced by close encounters with Ceres and Vesta (2011, unknown): “We note that the Lyapunov exponents LE0 computed in the absence of asteroid interactions are close to the values computed in a different way by Knežević & Milani (2003) and Novaković et al. (2011).”