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Table 3:

Ages, masses, and lithium abundances for the outliers in Fig. 5a.

Object
Age in Gyr mass in $M{_{\odot}}$ $\log\epsilon_{\rm Li}$ in dex Ages from other sources in Gyra
HD 221420 4.70 1.30 2.75 4.5 (GCS), 4.1 (VF05),
        5.1 (RP98)
HD 114613 6.03 1.19 2.69 5.1 (RP98), 5.6 (B07, rot),
        4.9 (VF05), 4.9 (RP98)
HD 2151 6.53 1.12 2.58 5.2 (GCS), 5.8 (VF05), 6.7 (V05)
HD 215456 8.36 1.04 2.38 7.3 (GCS), 7.0 (I02)
HD 32724 9.07 0.97 1.63 9.9 (GCS)
HD 4307 9.08 1.01 2.48 7.8 (W04, R'HK, rot),
        7.4 (GCS), 6.4 (VF05)
HD 78612 9.27 0.96 1.62 8.8 (GCS)
HD 114729 9.68 0.97 2.00 10.9 (GCS), 6.45 (RP98)
        [planet-host]
HD 145809 10.28 0.96 2.13 6.9 (W04, R'HK, rot),
        7.9 (GCS), 7.4 (VF05)
HD 32923 10.75 0.96 1.66 9.0 (VF05), 6.2 (W04),
        9.9 (GCS), >9.5 (S83)

Notes. R'HK denotes ages derived from chromospheric activity, rot denotes ages derived from rotation periods. (a) The abbreviations used here are the following: GCS: The Geneva-Copenhagen survey, Nordström et al. (2004), VF05: Valenti & Fischer (2005), RP98: Rocha-Pinto & Maciel (1998), V05: Vardavas (2005), I02: Ibukiyama & Arimoto (2002), W04: Wright et al. (2004) and S83: Soderblom (1983).


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