**Table 5:** Results of the mass determinations for (4) Vesta. Mean densities based on a IRAS diameter of $501~ {\rm km}$ are given in the third column. In the last column are presented correlation coefficients between the mass of Vesta and the mean motions of the perturbed asteroids.
Perturbed	Mass	Density	Correlation
asteroid	[ $10^{-10}~ M_{\odot}$ ]	[ ${\rm g~cm^{-3}}$ ]	coefficient
(3057) Malaren	$1.29\pm0.08$	$3.90\pm0.24$	-0.809
(5205) 1988CU7	$1.31 \pm 0.02$	$3.96\pm0.06$	0.829
(8331) Dawkins	$1.12\pm0.05$	$3.38\pm0.15$	0.753
(21225) 1995GQ1	$1.12\pm0.17$	$3.38\pm0.51$	-0.910

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