Table 1: Results obtained from least-square fitting of $\log\epsilon_{\rm nor}(X)$ vs. [Fe/H] of normal stars: $\log\epsilon_{\rm nor}(X)$ = A[Fe/H] + B; "cov'' is the covariance between A and B; "d.o.f.'' is the number of degrees of freedom.
X A B $\chi^2_{\rm red}$ cov (10^-4) d.o.f.

Sr 1.013 $\pm$ 0.024 2.908 $\pm$ 0.021 1.197 4.18 82

Y 1.112 $\pm$ 0.016 2.239 $\pm$ 0.013 1.002 1.58 160

Zr 0.939 $\pm$ 0.019 2.625 $\pm$ 0.015 1.385 2.06 66

Mo 0.970 $\pm$ 0.212 1.895 $\pm$ 0.342 1.472 715.2 7

Ba 0.992 $\pm$ 0.014 2.095 $\pm$ 0.011 1.978 1.07 214

La 1.190 $\pm$ 0.031 1.377 $\pm$ 0.039 4.891 10.91 47

Ce 1.009 $\pm$ 0.047 1.500 $\pm$ 0.047 0.923 20.20 34

Pr 0.867 $\pm$ 0.048 0.748 $\pm$ 0.050 1.180 19.99 13

Nd 0.950 $\pm$ 0.019 1.460 $\pm$ 0.017 1.635 2.46 99

Sm 0.811 $\pm$ 0.045 0.951 $\pm$ 0.045 1.407 18.76 34

Eu 0.783 $\pm$ 0.019 0.581 $\pm$ 0.015 1.263 2.20 165

Dy 0.840 $\pm$ 0.031 1.080 $\pm$ 0.044 4.312 11.70 22

**Table 1:** Results obtained from least-square fitting of $\log\epsilon_{\rm nor}(X)$ vs. [Fe/H] of normal stars: $\log\epsilon_{\rm nor}(X)$ = A[Fe/H] + B; "cov'' is the covariance between A and B; "d.o.f.'' is the number of degrees of freedom.
X	A	B	$\chi^2_{\rm red}$	cov (10^-4)	d.o.f.
Sr	1.013 $\pm$ 0.024	2.908 $\pm$ 0.021	1.197	4.18	82
Y	1.112 $\pm$ 0.016	2.239 $\pm$ 0.013	1.002	1.58	160
Zr	0.939 $\pm$ 0.019	2.625 $\pm$ 0.015	1.385	2.06	66
Mo	0.970 $\pm$ 0.212	1.895 $\pm$ 0.342	1.472	715.2	7
Ba	0.992 $\pm$ 0.014	2.095 $\pm$ 0.011	1.978	1.07	214
La	1.190 $\pm$ 0.031	1.377 $\pm$ 0.039	4.891	10.91	47
Ce	1.009 $\pm$ 0.047	1.500 $\pm$ 0.047	0.923	20.20	34
Pr	0.867 $\pm$ 0.048	0.748 $\pm$ 0.050	1.180	19.99	13
Nd	0.950 $\pm$ 0.019	1.460 $\pm$ 0.017	1.635	2.46	99
Sm	0.811 $\pm$ 0.045	0.951 $\pm$ 0.045	1.407	18.76	34
Eu	0.783 $\pm$ 0.019	0.581 $\pm$ 0.015	1.263	2.20	165
Dy	0.840 $\pm$ 0.031	1.080 $\pm$ 0.044	4.312	11.70	22

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