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Table A.1:

Cluster membership assessments for Jones & Prosser (1996) stars in our period sample.

Internala
JP96b Phota RVa Li Memc RV J97c RV Memd Va PM Probe
Identifier   Mem Mem J97 [km s-1] J97 [mag] JP96
F3_0172 JP 49 Y Ys ... ... ... 14.584 00%
F3_0176 JP 167 Y Ys ... ... ... 14.659 44%
F3_0215 JP 41 Y Ys ... ... ... 14.918 00%
F3_0258 JP 289 Y Ys Y -10.8 Y (47%) 15.236 76%
F3_0306 JP 265 Y Yb Y -17 Y ( 5%) 15.503 53%
F3_0320 JP 172 Y ... Y -9.8 Y (25%) 15.664 03%
F4_0136 JP 213 Y Ys Y -5.7 N ( 0%) 13.151 94%
F4_0169 JP 50 Y Ys ... ... ... 13.510 04%
F4_0194 JP 133 Y Ys Y -11.8 Y (77%) 13.662 96%
F4_0234 JP 148 Y Ys ... ... ... 13.959 05%
F4_0303 JP 227 Y Ys Y -15.4 Y (21%) 14.366 92%
F4_0317 JP 224 Y Ys Y -9.4 Y (18%) 14.410 91%
F4_0327 JP 199 Y Ys Y -9.0 Y (13%) 14.483 85%
F4_0335 JP 158 Y Yb Y -9.9 Y (26%) 14.546 86%
F4_0450 JP 113 Y Ys Y -13.5 Y (67%) 14.960 84%
F4_0667 JP 52 Y Yb ... ... ... 15.623 26%
F4_0695 JP 197 Y Ys ... ... ... 15.643 05%
F4_0730 JP 18 Y ... ... ... ... 15.741 36%
F4_0803 JP 229 Y Ys Y -9.9 Y (26%) 16.025 46%
F3_0121 JP 212 N ... ... ... ... 13.741 00%
F3_0163 JP 258 Y N ... ... ... 14.440 00%
F3_0165 JP 244 Y N ... ... ... 14.419 00%
F3_0388 JP 174 N ... ... ... ... 15.952 00%
F3_0413 JP 218 Y N ... ... ... 16.242 17%
F4_0167 JP 223 N ... ... ... ... 13.502 00%
F4_0404 JP 131 Y N ... ... ... 14.730 00%
F4_0515 JP 129 N ... ... ... ... 15.111 00%

Notes. (a) Data taken from Tables 2 and 3; (b) JP identifier from Jones & Prosser (1996); (c) cluster membership based on radial velocities and lithium 6708 Å equivalent widths, taken from Jones et al. (1997) [J97]; (d) radial velocity membership assessments are based on a Gaussian fit to the entire Jones et al. (1997) radial velocity sample (see also Fig. A.1); (e) proper motion membership probabilities are taken from JP96.


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