Table 3: Element abundances for the Sun in our analysis, in Anders & Grevesse (1989) and in Asplund et al. (2005).
El. No. $\log n$(X)$_{\odot}$ $\log n$(X)$_{\odot}$ $\log n$(X)$_{\odot}$
  lin. Our AG89 As05
Na  I 7 6.29 $\pm$ 0.05 6.33 6.17 $\pm$ 0.04
Mg  I 4 7.62 $\pm$ 0.14 7.58 7.53 $\pm$ 0.09
Al  I 3 6.33 $\pm$ 0.18 6.47 6.37 $\pm$ 0.06
Si  I 15 7.60 $\pm$ 0.03 7.55 7.51 $\pm$ 0.04
Ca  I 25 6.35 $\pm$ 0.04 6.36 6.31 $\pm$ 0.04
Ti  I 41 4.93 $\pm$ 0.03 4.99 4.90 $\pm$ 0.06
Ti  II 21 5.04 $\pm$ 0.04 - -
Cr  I 61 5.66 $\pm$ 0.03 5.67 5.64 $\pm$ 0.10
Cr  II 21 5.78 $\pm$ 0.02 - -
Fe  I 180 7.49 $\pm$ 0.04 7.52 7.45 $\pm$ 0.05
Fe  II 40 7.54 $\pm$ 0.03 - -
Ni  I 47 6.26 $\pm$ 0.02 6.28 6.23 $\pm$ 0.04
Ba  II - - 2.13 2.17 $\pm$ 0.07

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