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Table 2:

Final properties of the five selected generic models.
dSph # $L_{\rm {v}}$a $M/L_{\rm {V}}$b $M_{\rm {gas}}$c $\langle \rm {[Fe/H]}\rangle$d $\rm {[Fe/H]}<-3.0$e $\le $ $4~\rm {Gyr}$f $[4,8]~\rm {Gyr}$g $\ge $ $8~\rm {Gyr}$h
    $[10^6~{L_\odot}]$   $[10^8~ {M_\odot}]$ dex % % % %
Carina 533 0.72 231 0.28 -1.82 2.9 26.1 29.3 44.6
Leo II 587 0.97 219 0.33 -1.82 2.9 24.4 26.4 49.2
Sextans 590 0.53 390 0.17 -2.02 5.2 1.7 0.0 98.3
Sculptor 630 2.86 83 0.32 -1.82 5.6 3.6 0.0 96.4
Fornax 575 12.76 27 0.12 -1.03 1.2 14.4 10.6 75.0
a Stellar luminosity in V-band; b mass-to-light ratio; ac gas mass; d median of the metallicity distribution function; e fraction of stars having a metallicity lower than -3; f fraction of stars younger than $4~\rm {Gyr}$; g fraction of stars having ages between 4 and $8~\rm {Gyr}$; h fraction of stars older than $8~\rm {Gyr}$.


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