Table 1: Our sample stars in the giant, turnoff, and lower main-sequence regions. The Strömgren photometry is from Meibom (2000), B-V from Twarog et al. (1988), and (km s^-1) from Meibom et al. (2002).

Name	y	b-y	m1	c1	B-V
E12	10.324	0.661	0.465	0.314	1.126	1.1
E8	10.667	0.666	0.403	0.299	1.100	0.1
E60	10.870	0.673	0.491	0.312	1.141	1.9
E98	10.880	0.694	0.496	0.331	1.187	1.0
T812	11.059	0.648	0.413	0.344	1.140	0.5
E95	11.953	0.514	0.185	0.386	0.805	12.0
E3	12.051	0.374	0.169	0.527	0.612	29.9
E56	12.184	0.378	0.159	0.499	0.599	27.8
E19	12.240	0.412	0.157	0.484	0.651	32.1
E99	12.377	0.347	0.171	0.531	0.546	28.1
E17	12.625	0.337	0.158	0.543	0.539	10.0:
E25	12.654	0.365	0.118	0.552	0.537	21.3
E5	12.817	0.329	0.160	0.532	0.507	23.9
T1228	12.941	0.344	0.130	0.540	0.536	5.7
E14	13.119	0.335	0.154	0.507	0.516	34.1
E34	13.418	0.358	0.156	0.459	0.566	25.2
E15	13.515	0.374	0.146	0.447	0.563	10.0
E79	13.549	0.360	0.154	0.444	0.514	21.8
E64	13.722	0.370	0.160	0.430	0.594	9.2
E86	13.739	0.383	0.143	0.431	0.626	14.0
T2105	13.948	0.429	0.145	0.374	0.618	11.3
E7	14.165	0.402	0.179	0.368	0.643	2.1
E45	14.184	0.430	0.127	0.399	0.654	4.2