Astronomy & Astrophysics

Table 2: Possible values of the population parameters.
Parameter Possible values

M_y+i: $M_{\rm o}$ 0:1, 1:100, 1:30, 1:10, 1:3, 1:1, 3:1, 10:1, 1:0

${\rm age}_{y+i}$ 1, 2, 5, 10, 20, 50, 100, 200, 500 Myr

${\rm [Fe/H]}_{y+i}$ Taken from Cuisinier et al. (2004) or -1

${\rm age}_{\rm o}$ Fixed at 5 Gyr

${\rm [Fe/H]}_{\rm o}$ Fixed at -1.5

**Table 2:** Possible values of the population parameters.
Parameter	Possible values
M_y+i: $M_{\rm o}$	0:1, 1:100, 1:30, 1:10, 1:3, 1:1, 3:1, 10:1, 1:0
${\rm age}_{y+i}$	1, 2, 5, 10, 20, 50, 100, 200, 500 Myr
${\rm [Fe/H]}_{y+i}$	Taken from Cuisinier et al. (2004) or -1
${\rm age}_{\rm o}$	Fixed at 5 Gyr
${\rm [Fe/H]}_{\rm o}$	Fixed at -1.5

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