Table A.3.
[X/Fe] residuals of the depletion pattern fitting (see Figs. 7, A.4 and A.5). The values and uncertainties are obtained including MC simulations to take into account the dust depletion errors. We stress that the impact of dust depletion on the nuclear abundances is correlated between elements; i.e., a higher dust depletion correction lowers all [X/Fe] values except for [Al/Fe] which it raises, and vice-versa.
With α-element corr. | I | II | III | IV | V | VI | Tot |
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[C/Fe] |
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[O/Fe] |
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[Mg/Fe] |
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[Al/Fe] |
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[Si/Fe] |
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[S/Fe] |
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Without α-element corr. | I | II | III | IV | V | VI | Tot |
[C/Fe] |
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[O/Fe] |
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[Mg/Fe] |
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[Al/Fe] |
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[Si/Fe] |
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[S/Fe] |
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