**Table 4:** Mean abundances for the globular clusters NGC 104 (47 Tuc), NGC 6752, and NGC 6397.
Cluster ID	Type^a	N_*^b	[Fe/H]	${{\sigma}_{\rm Fe}}^{c}$	[Sr/Fe]	${{\sigma}_{\rm Sr}}^{c}$	[Y/Fe]	${{\sigma}_{\rm Y}}^{c}$	[Ba/Fe]	${{\sigma}_{\rm Ba}}^{c}$	[Eu/Fe]	${{\sigma}_{\rm Eu}}^{c}$
NGC 104 / 47 Tuc	SG	8	-0.69	0.06	+0.36	0.16	-0.11	0.10	+0.35	0.12	+0.17	...
	TO	3	-0.68	0.01	+0.28	0.14	+0.06	0.01	+0.22	0.12	+0.11	...
NGC 6397	SG	3	-2.08	0.01	-0.04	0.14	-0.20	0.09	-0.17	0.06	$\le$ +0.41	0.09
	TO	5	-2.07	0.01	-0.06	0.15	$\le$ -0.17	0.13	-0.31	0.06	$\le$ +0.46	...
Data for NGC 6752 (from James et al. 2004).
NGC 6752	SG	9	-1.49	0.07	-0.01	0.09	-0.01	0.13	+0.25	0.08	+0.40	0.09
	TO	9	-1.48	0.07	+0.12	0.19	-0.03	0.11	+0.11	0.09	+0.47	0.08

^a SG = subgiants, TO = turnoff stars; ^bN_* = number of stars in each group; ^c ${\sigma}_{\rm X}$ = standard deviation around the mean value.

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