Table 1: Main parameters for the models of the six dSph galaxies studied in this paper.
Galaxy $M_{\rm tot}^{\rm initial} (M_{\odot})$ w_i $\nu({\rm Gyr}^{-1})$ $\nu_1, \nu_2 ({\rm Gyr}^{-1})$ IMF

Sextans $5\times 10^{8}$ 9 0.08 0.01-0.3 Salpeter

Sculptor $5\times 10^{8}$ 13 0.2 0.05-0.5 Salpeter

Sagittarius $5\times 10^{8}$ 9 3.0 1.0-5.0 Salpeter

Draco $5\times 10^{8}$ 4 0.03 0.005-0.1 Salpeter

Ursa Minor $5\times 10^{8}$ 10 0.2 0.05-0.5 Salpeter

Carina $5\times 10^{8}$ 5 0.15 0.02-0.4 Salpeter

**Table 1:** Main parameters for the models of the six dSph galaxies studied in this paper.
Galaxy	$M_{\rm tot}^{\rm initial} (M_{\odot})$	w_i	$\nu({\rm Gyr}^{-1})$	$\nu_1, \nu_2 ({\rm Gyr}^{-1})$	IMF
Sextans	$5\times 10^{8}$	9	0.08	0.01-0.3	Salpeter
Sculptor	$5\times 10^{8}$	13	0.2	0.05-0.5	Salpeter
Sagittarius	$5\times 10^{8}$	9	3.0	1.0-5.0	Salpeter
Draco	$5\times 10^{8}$	4	0.03	0.005-0.1	Salpeter
Ursa Minor	$5\times 10^{8}$	10	0.2	0.05-0.5	Salpeter
Carina	$5\times 10^{8}$	5	0.15	0.02-0.4	Salpeter

Source LaTeX | All tables | In the text