**Table 16:** Comparison of copper abundances from our results and from other authors.
Star	$T_{\rm eff}$	$\log {g}$	$\xi_t$	[Fe/H]	[Cu/Fe]	[Cu/Fe] $_{\rm liter}$	Ref.
	(K)	(cm s^-2)	(km s^-1)
HD 92788	$5821\pm41$	$4.45\pm0.06$	$1.16\pm0.05$	$0.32\pm0.05$	$0.19 \pm 0.07$	0.52	1
HD 106252	$5899\pm35$	$4.34\pm0.07$	$1.08\pm0.06$	$-0.01\pm0.05$	$-0.02 \pm 0.07$	-0.04	1
HD 130322	$5392\pm36$	$4.48\pm0.06$	$0.85\pm0.05$	$0.03\pm0.04$	$0.03\pm0.07$	0.16	1
HD 134987	$5776\pm29$	$4.36\pm0.07$	$1.09\pm0.04$	$0.30\pm0.04$	$0.19 \pm0.06$	0.52	1
HD 141937	$5909\pm39$	$4.51\pm0.08$	$1.13\pm0.06$	$0.10\pm0.05$	$0.07\pm0.07$	0.13	1
HD 168746	$5601\pm33$	$4.41\pm0.12$	$0.99\pm0.05$	$-0.08\pm0.05$	$0.10 \pm0.07$	0.03	1
HD 187123	$5845\pm22$	$4.42\pm0.07$	$1.10\pm0.03$	$0.13\pm0.03$	$0.07\pm0.06$	0.20	1
HD 192263	$4947\pm58$	$4.51\pm0.20$	$0.86\pm0.09$	$-0.02\pm0.06$	$0.01 \pm0.08$	0.04	1

¹ From Sadakane et al. (2002).

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