Table A.2.
Standard deviation (σ) for [Fe/H] and [Mg/Fe] for all the groups with super-solar metallicity.
| Level 2 subgroup | Li detection | σ([Fe/H])tot | σ ([Fe/H])top6 | σ([Mg/Fe])tot | σ([Mg/Fe])top6 |
|---|---|---|---|---|---|
| G10 (purple) | LiD | 0.044 | 0.034 | 0.049 | 0.049 |
| LiUL | 0.047 | 0.076 | 0.064 | 0.047 | |
| G01 (green) | LiD | 0.047 | 0.034 | 0.072 | 0.085 |
| LiUL | 0.050 | 0.019 | 0.067 | 0.028 | |
| G02 (orange) | LiD | 0.038 | 0.038 | 0.058 | 0.054 |
| LiUL | 0.036 | 0.038 | 0.064 | 0.061 | |
| G03 (blue) | LiD | 0.050 | 0.019 | 0.043 | 0.038 |
| LiUL | 0.056 | 0.039 | 0.057 | 0.039 | |
Notes. The values are stratified by the type of Li detection and given both for the entire sample within the four groups and for the stars with the top 6 highest Li detection. The groups are listed in order of increasing ⟨[Fe/H]⟩. The Table is useful in order to evaluate the level of chemical homogeneity of the super-solar groups (Level 2 of the HC).
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