Table 1.
Parameters for the SFH, the IMF and the density laws of the seven model variants adopted from Mor et al. (2017).
| ID | SFH |
IMF |
Dens. law |
|||||
|---|---|---|---|---|---|---|---|---|
| γ (Gyr−1) | α1 | α2 | α3 | x1 | x2 | ρ⊙ (M⊙ pc−3) | hR (pc) | |
| DAV | 0.12 | 1.3 | 1.8 | 3.2 | 0.5 | 1.53 | 0.033 | 2170 |
| DM | 0.12 | 1.3 | 1.8 | 3.2 | 0.5 | 1.53 | 0.033 | 2530 |
| DBV | 0.12 | 1.3 | 1.8 | 3.2 | 0.5 | 1.53 | 0.039 | 2530 |
| DCV | 0.00 | 1.3 | 1.8 | 3.2 | 0.5 | 1.53 | 0.033 | 2530 |
| HRV | 0.12 | 1.6 | 1.6 | 3.0 | 0.5 | 1.00 | 0.033 | 2530 |
| HRVB | 0.12 | 1.6 | 1.6 | 3.0 | 0.5 | 1.00 | 0.039 | 2530 |
| SV | 0.12 | 2.35 | 2.35 | 2.35 | 0.5 | 1.53 | 0.033 | 2530 |
Notes. We show: (1) the three slopes of the initial mass function (α1,α2 and α3) and the two mass limits (x1 and x2) between the three truncated power laws of a Kroupa-like type; (2) the stellar volume mass density at the position of the Sun ( ρ⊙); and (3) the radial scale length of the old thin disc (hR).
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