Table 1: Stars with planets considered in this study.
Id [Fe/H] $T_{\rm eff}$ [$\alpha $/Fe] Age V
HIP dex K dex Gyr km-1
3479 -0.24 5626 0.04   -4
3497 -0.33 5636 0.19 11.5 (6.5, 16.1) -109
5054 -0.52 5835 0.188 10.4 (5.6, 14.8) -67
10138 -0.24 5163 0.075   -75
26381 -0.38 5546 0.138 14.7 (8.2, 20.0) -24
31688 -0.54 4554 0.19 9.3 (7.4, 11.2)  
58952 -0.28 4773 0.163   -8
62534 -0.36 5494 0.17 12.0 (4.3 19.5) -86
64426 -0.70 5884 0.198 12.4 (9.5, 15.0) -69
64459 -0.25 5886 0.047 8.2 (6.3, 10.0) -86
78459 -0.21 5853 0.07 8.5 (5.8, 10.7) -36
83949 -0.67 5868 0.18   -53
98714 -0.26 5327 0.03 5.3 (4.5, 6.3) -48
HD 171028 -0.49 5663 0.05   2
Notes: Atmospheric parameters from Gilli et al. (2006) or Soubiran & Girard (2005) for HIP 3497 and HIP 83949. V velocities from Nordström et al. (2004). Ages are derived as described in the text, except for HIP 31688, which age comes from da Silva et al. (2006). The ages of HIP 58952 (giant), HIP 3479 and HIP 10138 could not be determined. Parameters of HD 171028 from Santos et al. (2007) are given.

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