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Table 3

Stellar parameters and obtained iron abundances, [Fe/H], for selected stars.

Object Teff, K log    g Ref. Vmic1 Ion N2 Iron abundances, [Fe/H]

LTE SH = 0 SH = 0.1 SH = 1
1 2 3 4 5 6 7 8 9 10 11

Sun3 5777 4.44 0.9 Fe i 54   7.53 ± 0.09   7.61 ± 0.10   7.56 ± 0.09   7.54 ± 0.09
Fe ii 18   7.56 ± 0.05   7.55 ± 0.05   7.56 ± 0.05   7.56 ± 0.05
HD 10700 5377 4.53 DTK04 0.8 Fe i 39 −0.49 ± 0.02 −0.44 ± 0.03 −0.49 ± 0.02 −0.49 ± 0.03
(τ Cet) Fe ii 13 −0.52 ± 0.04 −0.52 ± 0.04 −0.52 ± 0.04 −0.52 ± 0.04
HD 61421 6510 ± 49 3.96 ± 0.02 AP02 1.8 Fe i 45 −0.12 ± 0.07 −0.12 ± 0.07 −0.10 ± 0.07 −0.13 ± 0.07
(Procyon) Fe ii 15 −0.03 ± 0.05 −0.03 ± 0.05 −0.04 ± 0.05 −0.03 ± 0.05
HD 84937 6350 ± 37 4.09 ± 0.05 IRFM+Hip 1.7 Fe i 21 −2.17 ± 0.07 −1.96 ± 0.06 −2.00 ± 0.07 −2.13 ± 0.07
Fe ii 9 −2.08 ± 0.04 −2.06 ± 0.03 −2.08 ± 0.04 −2.08 ± 0.04
HD 102870 6060 ± 49 4.11 ± 0.01 NDR09 1.2 Fe i 39   0.11 ± 0.03   0.11 ± 0.04   0.13 ± 0.04   0.11 ± 0.03
(β Vir) Fe ii 13   0.22 ± 0.04   0.23 ± 0.04   0.22 ± 0.04   0.22 ± 0.04
HD 122563 4600 ± 61 1.60 ± 0.07 IRFM+Hip 1.95 Fe i 35 −2.77 ± 0.11 −2.42 ± 0.09 −2.61 ± 0.09 −2.74 ± 0.10
Fe ii 15 −2.56 ± 0.07 −2.45 ± 0.12 −2.56 ± 0.07 −2.56 ± 0.07

Notes.

1

Microturbulence velocity is given in km s-1.

2

Number of lines used.

3

We present the absolute iron abundances for the Sun calculated using the gf-values from Table 5. References to the adopted Teff and log    g: DTK04 = Di Folco et al. (2004), AP02 = Allende Prieto et al. (2002), NDR09 = North et al. (2009), IRFM+Hip = IRFM temperature and Hipparcos-parallax based log    g.

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