Table 4
Recommended abundances of SMSS0313-6708, with statistical and systematic uncertainties.
| Species | A(X) | [X/H] | σstat | σsys a | Source |
|
|
|||||
| Li i | 0.82 | −0.23 | 0.08 | 0.10 | * |
| C (CH) | 5.88 | −2.55 | 0.09 | 1 | |
| N (NH) | < 3.13 | <−4.70 | 0.3 | 1 | |
| O (OH) | 6.16 | −2.53 | 0.15 | 1 | |
| Na i | < 0.64 | <−5.60 | 0.10 | 0.08 | * |
| Mg i | 3.77 | −3.83 | 0.03 | 0.10 | * |
| Al i | < 0.79 | <−5.66 | 0.25 | 0.11 | * |
| Si i | < 1.91 | <−5.60 | 0.3 | 2 | |
| Ca ii | −0.60 | −6.94 | 0.06 | 0.10 | * |
| Sc ii | < −2.35 | <−5.50 | 0.3 | 2 | |
| Ti ii | < −2.15 | <−7.10 | 0.3 | 2 | |
| V ii | < −0.37 | <−4.30 | 0.3 | 2 | |
| Cr i | < −0.66 | <−6.30 | 0.3 | 2 | |
| Mn i | < −0.37 | <−5.80 | 0.3 | 2 | |
| Fe ib | <0.50 | <−7.00 | 0.24 | 0.16 | * |
| Co i | < −0.41 | <−5.40 | 0.3 | 2 | |
| Ni i | < −0.68 | <−6.90 | 0.3 | 2 | |
| Cu i | < −1.31 | <−5.50 | 0.3 | 2 | |
| Zn i | <1.16 | <−3.40 | 0.3 | 2 | |
| Sr ii | < −4.03 | <−6.90 | 0.3 | 2 | |
| Ba ii | < −3.92 | <−6.10 | 0.3 | 2 | |
| Eu ii | < −2.38 | <−2.90 | 0.3 | 2 | |
Notes. Uncertainties and upper limits are given at the 1σ level.
Systematic uncertainty due to uncertainties in stellar parameters, estimated by Keller et al. (2014) as σ(Teff) = 100 K and σ(log g) = 0.2 dex.
Reference. (*) This work, 3D NLTE; (1) Bessell et al. (2015), 3D LTE analysis of molecular lines; (2) Bessell et al. (2015), 1D LTE analysis.
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