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Table B.1

Derived elemental abundances for J0040+2729.

N log ϵ(X) [X/H] σ[X/H] [X/Fe] σ[X/Fe]
C-H 12 5.55 −2.81 0.18 +0.02 0.18
Ccorr +0.56
OI 1 6.46 −2.23 0.30 +0.60 0.29
NaI 2 3.67 −2.56 0.31 +0.26 0.31
MgI 5 5.25 −2.35 0.14 +0.47 0.14
AlI 2 3.04 −3.37 0.24 −0.55 0.25
SiI 2 5.15 −2.45 0.30 +0.37 0.30
KI 2 2.98 −2.02 0.26 +0.81 0.26
CaI 18 3.90 −2.43 0.14 +0.40 0.14
ScI 1 0.30 −2.85 0.48 −0.03 0.48
ScII 9 0.45 −2.72 0.15 −0.05 0.12
TiI 15 2.34 −2.67 0.20 +0.15 0.20
TiII 25 2.46 −2.35 0.18 +0.32 0.14
VI 3 1.02 −2.91 0.14 −0.09 0.14
VII 8 1.40 −2.49 0.11 +0.18 0.14
CrI 6 2.63 −2.94 0.21 −0.11 0.21
CrII 4 2.94 −2.70 0.14 −0.03 0.12
MnI 6 2.14 −3.22 0.15 −0.39 0.15
FeI 109 4.77 −2.83 0.11 0.00 0.10
FeII 14 4.78 −2.67 0.14 0.00 0.10
CoI 6 2.16 −2.81 0.16 +0.02 0.16
NiI 15 3.52 −2.80 0.15 +0.03 0.15
ZnI 2 2.02 −2.55 0.25 +0.27 0.25
SrII 2 0.32 −2.53 0.26 +0.15 0.27
YII 21 −0.36 −2.54 0.11 +0.14 0.14
ZrII 15 0.35 −2.20 0.12 +0.48 0.14
MoI 1 −0.18 −2.06 0.23 +0.76 0.24
RuI 1 0.14 −1.61 0.34 +1.22 0.34
BaII 5 −0.19 −2.30 0.19 +0.38 0.16
LaII 27 −0.89 −2.01 0.12 +0.66 0.14
CeII 35 −0.57 −2.15 0.11 +0.53 0.14
PrII 12 −1.08 −1.72 0.13 +0.95 0.14
NdII 64 −0.44 −1.86 0.10 +0.81 0.14
SmII 46 −0.78 −1.73 0.10 +0.95 0.14
EuII 6 −1.10 −1.67 0.15 +1.00 0.13
GdII 13 −0.65 −1.71 0.11 +0.96 0.14
TbII 3 −1.40 −1.47 0.16 +1.21 0.14
DyII 10 −0.48 −1.62 0.12 +1.05 0.14
HoII 4 −1.23 −1.74 0.21 +0.94 0.17
ErII 6 −0.79 −1.72 0.14 +0.96 0.15
TmII 4 −1.54 −1.53 0.19 +1.14 0.16
YbII 1 −0.88 −1.72 0.24 +0.95 0.25
LuII 1 −1.50 −1.60 0.32 +1.07 0.30
HfII 2 −0.84 −1.73 0.24 +0.95 0.27
OsI 1 −0.20 −1.60 0.25 +1.22 0.26
IrI 1 −0.26 −1.64 0.36 +1.18 0.35
ThII 1 −1.52 −1.54 0.28 +1.14 0.25

Notes. For each element and star, we report: the number of spectral lines used (N), the logarithmic abundance log ϵ(X), the abundance relative to hydrogen [X/H], its uncertainty σ[X/H], the abundance relative to iron [X/Fe], and the corresponding uncertainty σ[X/Fe]. Reported values include both detections and upper limits, the latter indicated with a “<” symbol. All abundances listed in this table are 1D and LTE. Data for the remaining stars are provided in the CDS.

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