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Table 4.

Final adopted abundances.

LTE
 NLTE
X ⟨log ϵ(X)⟩ (a) [X/Fe] (b) n ⟨log ϵ(X)⟩ (a) [X/Fe] n log ϵ(X)⊙(c)
[dex] [dex] [dex] [dex] [dex]
Li I <−0.34 <0.41 1 ... ... ... 1.05
C (CH) 6.25 ± 0.05 −0.38 ± 0.07 1 ... ... ... 8.43
N (NH) 6.21 ± 0.10 0.18 ± 0.11 1 ... ... ... 7.83
O I 7.79 ± 0.18 0.70 ± 0.18 2 7.79 ± 0.18 0.70 ± 0.18 2 8.69
Na I 4.50 ± 0.10 0.06 ± 0.11 2 4.42 ± 0.10 −0.14 ± 0.12 2 6.24
Mg I 6.25 ± 0.10 0.45 ± 0.11 3 6.24 ± 0.10 0.32 ± 0.12 3 7.60
Al I 4.54 ± 0.15 −0.11 ± 0.16 5 4.68 ± 0.06 −0.09 ± 0.09 5 6.45
Si I 6.21 ± 0.13 0.50 ± 0.14 16 6.23 ± 0.03 0.40 ± 0.08 5 7.51
Si II 6.49 ± 0.10 0.58 ± 0.10 2 ... ... ... 7.51
S I 6.03 ± 0.04 0.71 ± 0.06 4 ... ... ... 7.12
K I 4.15 ± 0.10 0.92 ± 0.11 2 3.60 ± 0.10 0.25 ± 0.12 2 5.03
Ca I 4.92 ± 0.06 0.38 ± 0.08 25 ... ... ... 6.34
Sc II 1.66 ± 0.06 0.11 ± 0.06 11 ... ... ... 3.15
Ti I 3.34 ± 0.10 0.19 ± 0.11 20 3.81 ± 0.10 0.54 ± 0.13 15 4.95
Ti II 3.67 ± 0.10 0.31 ± 0.10 28 ... ... ... 4.95
V I 2.07 ± 0.12 −0.06 ± 0.13 4 ... ... ... 3.93
V II 2.50 ± 0.10 0.16 ± 0.10 2 ... ... ... 3.93
Cr I 3.67 ± 0.12 −0.17 ± 0.13 12 ... ... ... 5.64
Cr II 4.25 ± 0.15 0.21 ± 0.15 15 ... ... ... 5.64
Mn I 3.33 ± 0.08 −0.30 ± 0.10 4 3.73 ± 0.08 −0.02 ± 0.11 4 5.43
Fe I 5.70 ± 0.07 0.00 ± 0.09 133 5.82 ± 0.10 0.00 ± 0.13 133 7.50
Fe II 5.90 ± 0.03 0.00 ± 0.04 13 5.90 ± 0.03 0.00 ± 0.04 13 7.50
Co I 3.25 ± 0.11 0.06 ± 0.12 6 3.61 ± 0.10 0.30 ± 0.12 3 4.99
Ni I 4.43 ± 0.07 0.01 ± 0.09 32 ... ... ... 6.22
Cu I 1.76 ± 0.10 −0.63 ± 0.11 3 ... ... ... 4.19
Zn I 2.88 ± 0.10 0.12 ± 0.11 2 ... ... ... 4.56
Ga I 1.03 ± 0.20 −0.21 ± 0.21 1 ... ... ... 3.04
Rb I < 1.52 < 0.45 1 ... ... ... 2.87
Sr I 1.00 ± 0.10 −0.07 ± 0.11 1 1.40 ± 0.10 0.21 ± 0.12 1 2.87
Sr II 1.50 ± 0.26 0.23 ± 0.26 1 ... ... ... 2.87
Y II 0.54 ± 0.09 −0.07 ± 0.09 7 ... ... ... 2.21
Zr II 1.26 ± 0.09 0.28 ± 0.09 5 1.41 ± 0.10 0.42 ± 0.10 2 2.58
Mo I 0.48 ± 0.10 0.40 ± 0.11 1 ... ... ... 1.88
Ru I 0.55 ± 0.10 0.60 ± 0.11 1 ... ... ... 1.75
Rh I −0.19 ± 0.40 0.70 ± 0.40 1 ... ... ... 0.91
Pd I −0.12 ± 0.20 0.11 ± 0.21 1 ... ... ... 1.57
Ag I −0.29 ± 0.20 0.57 ± 0.21 1 ... ... ... 0.94
Ba II 0.93 ± 0.10 0.35 ± 0.10 2 0.74 ± 0.10 0.16 ± 0.10 2 2.18
La II −0.09 ± 0.06 0.41 ± 0.06 6 ... ... ... 1.10
Ce II 0.19 ± 0.03 0.21 ± 0.04 11 ... ... ... 1.58
Pr II −0.35 ± 0.10 0.53 ± 0.10 3 ... ... ... 0.72
Nd II 0.21 ± 0.06 0.39 ± 0.06 22 ... ... ... 1.42
Sm II −0.06 ± 0.04 0.58 ± 0.05 12 ... ... ... 0.96
Eu II −0.35 ± 0.10 0.73 ± 0.10 3 ... ... ... 0.52
Gd II 0.04 ± 0.15 0.56 ± 0.15 5 ... ... ... 1.07
Tb II −0.74 ± 0.10 0.55 ± 0.10 2 ... ... ... 0.30
Dy II 0.21 ± 0.07 0.70 ± 0.07 4 ... ... ... 1.10
Ho II −0.49 ± 0.10 0.63 ± 0.10 2 ... ... ... 0.48
Er II −0.04 ± 0.09 0.64 ± 0.09 4 ... ... ... 0.92
Tm II −0.87 ± 0.00 0.63 ± 0.02 4 ... ... ... 0.10
Yb II −0.06 ± 0.20 0.70 ± 0.20 1 ... ... ... 0.84
Lu II −0.57 ± 0.10 0.93 ± 0.10 1 ... ... ... 0.10
Hf II −0.23 ± 0.10 0.52 ± 0.10 3 ... ... ... 0.85
Os I 0.40 ± 0.10 0.80 ± 0.11 2 ... ... ... 1.40
Ir I 0.42 ± 0.10 0.84 ± 0.11 1 ... ... ... 1.38
Pb I < 0.37 < 0.42 1 ... ... ... 1.75 (d)
Th II −0.85 ± 0.10 0.73 ± 0.10 1 ... ... ... 0.02
U II <  − 1.21 < 0.93 1 ... ... ... −0.54

Notes.

(a)

For n ≥ 4, the error is considered as the mad of the line-by-line abundance distribution scaled by the factor 1.48 to be concordant with a normal distribution. Otherwise, a floor error of 0.10 dex is assumed (see main text for details).

(b)

With the exception of O I, [X/Fe]LTE is given relative to the LTE abundance of the Fe species at the same ionization stage.

(c)

The solar reference abundances are from Asplund et al. (2009).

(d)

The Pb abundance was taken from meteoroids.

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