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Table 3

Stellar abundances [X/H] of HIP 100963 relative to the Sun and corresponding errors.

Element [X/H] ΔTeff Δlog g Δvt Δ[Fe/H] Parama obs.b Totalc [X/H]d
LTE ±4 K ± 0.01 dex ±0.01 km s-1 ±0.004 dex GCE
(dex) (dex) (dex) (dex) (dex) (dex) (dex) (dex) (dex)
C –0.066 0.002 0.003 0.000 0.000 0.004 0.018 0.018 0.015
O –0.036 0.004 0.002 0.001 0.000 0.005 0.006 0.008 0.038
Na –0.067 0.002 0.001 0.000 0.000 0.002 0.006 0.006 0.008
Mg –0.024 0.004 0.001 0.002 0.001 0.005 0.007 0.008 0.022
Al –0.037 0.002 0.000 0.000 0.000 0.002 0.006 0.006 –0.006
Si –0.021 0.001 0.001 0.000 0.001 0.002 0.005 0.005 0.004
Ca 0.010 0.003 0.001 0.002 0.001 0.004 0.006 0.007 –0.009
Sc* –0.020 0.000 0.004 0.002 0.001 0.005 0.004 0.006 0.048
Ti* 0.003 0.000 0.005 0.002 0.001 0.005 0.006 0.008 0.028
V –0.018 0.004 0.001 0.000 0.000 0.004 0.006 0.007 0.002
Cr* 0.012 0.001 0.004 0.002 0.001 0.005 0.006 0.008 0.002
Mn –0.027 0.003 0.000 0.001 0.001 0.003 0.006 0.007 0.021
Fe* –0.003 0.003 0.000 0.002 0.001 0.004 0.001 0.004 –0.003
Co –0.046 0.003 0.002 0.000 0.000 0.004 0.011 0.012 0.017
Ni –0.025 0.002 0.000 0.002 0.001 0.003 0.006 0.007 0.024
Cu –0.056 0.002 0.001 0.002 0.001 0.003 0.009 0.010 0.027
Zn –0.033 0.000 0.001 0.002 0.001 0.002 0.007 0.007 0.033
Sr 0.055 0.004 0.001 0.001 0.001 0.004 0.007 0.008 ...
Y 0.065 0.001 0.005 0.004 0.002 0.007 0.008 0.010 ...
Zr 0.074 0.001 0.005 0.002 0.001 0.006 0.006 0.008 ...
Ba 0.051 0.001 0.001 0.004 0.002 0.005 0.008 0.009 ...
La 0.072 0.001 0.006 0.000 0.001 0.006 0.011 0.013 ...
Ce 0.054 0.001 0.005 0.001 0.002 0.006 0.007 0.009 ...
Nd 0.066 0.001 0.006 0.000 0.002 0.006 0.006 0.009 ...
Sm 0.086 0.001 0.005 0.001 0.001 0.005 0.007 0.009 ...
Eu 0.069 0.001 0.006 0.001 0.001 0.006 0.007 0.009 ...

Notes.

(a)

Adding errors in stellar parameters.

(b)

Observational errors.

(c)

Total errors (stellar and observational parameters).

(d)

Abundances corrected by subtracting the chemical evolution of the Galactic thin disk.

(*)

The errors due to uncertainties in the stellar parameters come from ScII, TiII, CrII, and FeI.

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