Table B.2
NLTE abundance corrections.
| Star | [Sr II/Fe] LTE | [Ba II/Fe] LTE | [Eu II/Fe] LTE | [Sr II/Fe] NLTE,corr | [Ba II/Fe] NLTE,corr | [Eu II/Fe] NLTE,corr | [Sr II/Fe] corrected | [Ba II/Fe] corrected | [Eu II/Fe] corrected |
|---|---|---|---|---|---|---|---|---|---|
| J0040+2729 | 0.15 | 0.38 | 1.00 | −0.06 | −0.28 | 0.01 | 0.09 | 0.10 | 1.01 |
| J0217-1903 | 0.68 | 0.65 | 1.57 | − | −0.19 | − | − | 0.46 | − |
| J0246–1518 | 0.48 | 0.78 | 1.43 | −0.07 | −0.14 | −0.01 | 0.41 | 0.64 | 1.42 |
| J1430–2317 | 0.15 | 0.05 | 0.62 | − | −0.14 | − | − | −0.09 | − |
| J1432–4125 | 0.49 | 0.86 | 1.49 | − | −0.19 | −0.02 | − | 0.67 | 1.47 |
| J1916–5544 | 0.19 | 0.11 | 0.81 | 0.08 | −0.20 | 0.02 | 0.27 | −0.09 | 0.83 |
| J2009–3410 | 0.19 | 0.18 | 1.20 | −0.07 | −0.15 | − | 0.12 | 0.03 | − |
| J2049–5124 | −0.47 | −0.14 | 0.39 | − | −0.25 | 0.09 | − | −0.39 | 0.48 |
| J2106–6828 | 0.51 | 0.52 | 1.10 | 0.03 | −0.24 | − | 0.54 | 0.28 | − |
| J2109–1310 | 0.22 | 0.51 | 1.06 | 0.03 | −0.34 | −0.01 | 0.25 | 0.17 | 1.05 |
Notes. Corrections were calculated for Sr II (Mashonkina et al. 2022), Ba II (Mashonkina & Belyaev 2019) and Eu II (Mashonkina & Gehren 2000). Column 1 lists the star identifier. Columns 2–4 give the LTE abundances [Sr II/Fe], [Ba II/Fe], and [Eu II/Fe]. Columns 5–7 list the NLTE corrections applied to Sr, Ba, and Eu. Columns 8–10 show the resulting NLTE-corrected abundances. These corrections are based on literature values for stars where NLTE effects have been quantified.
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