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Table 5

Abundance sensitivities.

HIP 23311 HIP 77408
Ion
Δ T eff Δ log g Δ ξ t Δ T eff Δ log g Δ ξ t
±43 ±0.11 ±0.41 ±25 ±0.06 ±0.17
(K) (cm s-2) (km s-1) (K) (cm s-2) (km s-1)

C I 0.06 0.03 <0.01 0.02 0.02 <0.01
O I 0.07 0.03 0.01 0.03 0.02 0.01
Na I 0.04 0.04 0.04 0.02 0.01 0.01
Mg I 0.01 0.02 0.03 0.01 0.01 0.02
Al I 0.02 0.02 0.04 0.01 <0.01 0.01
Si I 0.02 0.02 0.01 0.01 0.01 0.01
S I 0.05 0.03 <0.01 0.02 0.02 <0.01
Ca I 0.04 0.03 0.05 0.02 0.02 0.03
Sc I 0.05 0.02 0.09 0.03 <0.01 0.01
Sc II 0.01 0.04 0.06 <0.01 0.02 0.03
Ti I 0.05 0.03 0.10 0.03 <0.01 0.04
Ti II 0.01 0.04 0.06 <0.01 0.02 0.03
V I 0.06 0.02 0.09 0.03 <0.01 0.01
Cr I 0.03 0.02 0.07 0.02 0.01 0.03
Cr II 0.03 0.04 0.05 0.01 0.02 0.03
Mn I 0.02 0.03 0.07 0.02 <0.01 0.04
Co I <0.01 0.04 0.01 0.01 0.01 <0.01
Ni I <0.01 0.01 0.05 0.01 0.01 0.02
Cu I 0.02 0.03 0.04 <0.01 0.02 <0.01
Zn I 0.02 0.01 0.06 0.01 0.01 0.03

HIP 113044 HIP 28767
Ion
Δ T eff Δ log g Δ ξ t Δ T eff Δ log g Δ ξ t
±20 ±0.05 ±0.12 ±25 ±0.05 ±0.16
(K) (cm s-2) (km s-1) (K) (cm s-2) (km s-1)

C I 0.01 0.01 <0.01 0.01 0.01 <0.01
O I 0.02 0.02 0.02 0.01 0.01 0.01
Na I 0.01 0.01 0.01 0.01 0.01 0.01
Mg I 0.01 0.01 0.02 0.01 0.01 0.02
Al I 0.01 <0.01 0.01 0.01 <0.01 0.01
Si I <0.01 <0.01 0.01 0.01 <0.01 0.01
S I 0.01 0.01 0.01 0.01 0.01 0.01
Ca I 0.01 0.01 0.03 0.02 0.01 0.03
Sc I 0.02 <0.01 <0.01 0.02 <0.01 <0.01
Sc II <0.01 0.02 0.03 <0.01 0.02 0.03
Ti I 0.02 <0.01 0.01 0.02 <0.01 0.01
Ti II <0.01 0.02 0.03 <0.01 0.02 0.04
V I 0.02 <0.01 <0.01 0.02 <0.01 <0.01
Cr I 0.01 <0.01 0.02 0.02 <0.01 0.03
Cr II 0.01 0.02 0.04 <0.01 0.02 0.05
Mn I 0.01 <0.01 0.03 0.02 <0.01 0.03
Co I 0.02 <0.01 <0.01 0.02 <0.01 <0.01
Ni I 0.01 <0.01 0.02 0.02 <0.01 0.01
Cu I 0.01 <0.01 <0.01 0.01 <0.01 <0.01
Zn I <0.01 <0.01 0.04 0.01 0.01 0.04

Notes. The changes in the derived abundances when each stellar parameter is perturbed by its corresponding uncertainty are given.

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