All Tables

Table 1: Numerical values of the coefficients used to regularize g as a function of n for the Vesta family (s-intervals between -42.89 and -45.00''/yr, and between -45.00 and -47.64''/yr).
Table 2: Numerical values of the coefficients used to regularize g as a function of e for the Hansa family.
Table 3: The limits in the $(a,e,\sin(i))$ domain of the local background for the families studied in this paper.
Table 4: Percentage of resonant asteroids in the local background identified as family members by the classical method (CHCM), the ``standard'' frequency method (FHCM), and the new distance metrics introduced in this article (AHCM).