Table 3: Same as Table 2 but for the important lines in the Keck I/HIRES spectrum.

Species		 $\lambda$ (Å) $\chi$ (eV) $\log gf$ [X/H] Species $\lambda$ (Å) $\chi$ (eV) $\log gf$ [X/H]

Mg  I		 7875.434 5.932 -2.13 - O  I 7775.400 9.110 0.10 -
Mg  II 7877.054 9.996 0.39 0.75 O  I 8446.249 9.521 -0.46 -
Mg  I 7877.478 5.932 -1.95 - O  I 8446.359 9.521 0.23 1.80
Mg  I 7881.669 5.933 -1.51 0.70 O  I 8446.759 9.521 0.01 -
Mg  I 8712.676 5.932 -1.67 - S  I 8693.137 7.870 -1.37 -
Mg  I 8712.689 5.932 -1.37 0.60 S  I 8693.931 7.870 -0.51 0.90
Mg  I 8717.803 5.933 -2.85 - S  I 8694.626 7.870 0.08 -
Mg  I 8717.816 5.933 -1.85 - Si  I 8646.371 6.206 -1.94 -
Mg  I 8717.825 5.933 -0.93 0.65 Si  I 8648.465 6.206 -0.30 0.55
Mg  I 8736.006 5.946 -1.93 - Si  I 8728.010 6.181 -0.61 0.60
Mg  I 8736.019 5.946 -0.69 0.65 Si  I 8728.594 6.181 -1.72 -
Mg  I 8736.019 5.946 -1.97 - Si  I 8729.282 6.181 -2.30 -
Mg  I 8736.029 5.946 -1.02 - Ti  I 8434.957 0.848 -0.88 0.35
O  I 7771.960 9.110 0.45 2.00 Ti  I 8435.652 0.836 -1.02 -
O  I 7774.180 9.110 0.31 - Ti  I 8438.923 2.256 -0.79 -


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