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Table 1

Differential abundances of HIP 114328 relative to the Sun and errors.

Element LTE ΔTeff Δlog g Δvt Δ[Fe/H] Parama Obsb Totalc
+10 K +0.03 dex +0.03 km s-1 +0.01 dex
(dex) (dex) (dex) (dex) (dex) (dex) (dex) (dex)
C 0.009 −0.005 0.007 0.000 -0.001 0.009 0.009 0.012
N 0.003 0.013 0.007 0.020 0.009 0.026 0.001 0.026
Na 0.007 0.005 −0.001 0.000 0.001 0.005 0.005 0.007
Mg 0.019 0.005 −0.006 −0.004 0.000 0.009 0.001 0.009
Al −0.002 0.005 −0.001 −0.001 0.001 0.005 0.009 0.010
Si 0.006 0.002 0.001 −0.001 0.001 0.003 0.004 0.005
S 0.015 −0.004 0.006 0.000 0.000 0.007 0.004 0.008
Ca −0.013 0.007 -0.005 −0.005 0.001 0.010 0.003 0.010
Sc 0.017 0.008 0.002 −0.001 0.001 0.008 0.006 0.010
Ti −0.016 0.004 0.005 −0.005 −0.002 0.008 0.003 0.009
V −0.003 0.010 0.001 −0.002 0.001 0.010 0.005 0.011
Cr −0.022 −0.002 0.010 −0.004 0.002 0.011 0.004 0.012
Mn −0.013 0.008 −0.004 -0.007 0.002 0.012 0.006 0.013
Fe -0.022 0.001 0.005 −0.006 0.002 0.008 0.004 0.009
Co -0.010 0.008 0.003 −0.002 0.001 0.009 0.005 0.010
Ni -0.014 0.006 0.000 −0.005 0.002 0.008 0.002 0.008
Cu 0.024 0.006 −0.001 −0.007 0.003 0.010 0.001 0.010
Zn 0.005 0.001 0.002 −0.006 0.003 0.007 0.010 0.012

Notes. Abundances of V, Mn, Co, and Cu account for HFS.

(a)

Adding errors in stellar parameters.

(b)

Observational errors.

(c)

Total errors (stellar parameters and observational).

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