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Table 4.
Iron abundance ranges, and coefficients m and q of the linear law [El/Fe] = m ⋅ [Fe/H] + q that express the chemical abundances used to synthesize the spectra of the three mock stellar populations.
| Mock | [Fe/H] range | C, N, O |
Mg |
Al, Si, Ca, Ti |
Sc |
Mn |
Zn |
Ba |
|||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| population | (dex) | m | q | m | q | m | q | m | q | m | q | m | q | m | q |
| Thin disk | 0.0 ≤[Fe/H]≤ + 0.2 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 | 0.25 | 0.0 | 0.4 | 0.0 | 0.5 | 0.0 | −0.5 | 0.0 |
| stars | −0.8 <[Fe/H]< 0.0 | −0.4 | 0.0 | −0.3 | 0.0 | −0.15 | 0.0 | 0.0 | 0.0 | 0.4 | 0.0 | −0.2 | 0.0 | 0.2 | 0.0 |
| Halo/thick disk | −1.0 <[Fe/H]< − 0.2 | −0.5 | +0.1 | −0.3 | +0.1 | −0.2 | +0.1 | −0.2 | 0.0 | 0.4 | 0.0 | −0.2 | 0.0 | 0.2 | 0.0 |
| stars | −2.2 ≤[Fe/H]≤ − 1.0 | 0.0 | +0.6 | 0.0 | +0.4 | 0.0 | +0.3 | 0.0 | 0.2 | 0.0 | −0.4 | 0.0 | 0.2 | 0.0 | −0.2 |
| Accreted stars | −2.2 ≤[Fe/H]≤ −1.0 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 | −0.4 | 0.0 | 0.0 | 0.0 | 0.0 |
Notes. Any element not reported has m = 0, q = 0.
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