All Tables

Table 1: Parameters of the Gaussians fitting the U distribution of stars from Famaey et al. (2005), in the V-strip corresponding to the Pleiades, $-28 \le V$ (km s^-1) $\le$ -18. The parameters k_i give the relative fractions $N_i/N_{\rm tot}$ , where N_i is the total number of stars in component i, and $N_{\rm tot}=1176$ is the total number of stars in the V-strip. The fraction f_s is the relative fraction of stars from the Pleiades moving group with respect to all stars in the restricted $\pm$ $1.4 \sigma _{U}$ range around the Gaussian average, corresponding to the Pleiades zone where the wavelet coefficients are nonzero at scale 4 (see Sect. 3).
Table 2: Same as Table 1 in the V-strip corresponding to the Hyades, $-24 \le V$ (km s^-1) $\le$ -12, with $N_{\rm tot} = 1487$ .
Table 3: Same as Table 1 in the V-strip corresponding to the Sirius moving group, $-5 \le V$ (km s^-1) $\le$ 8, with $N_{\rm tot} = 1071$ .