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Table 5

Li abundances for planet hosts not belonging to the HARPS-GTO sample.

Star T eff log g ξ t [Fe/H] Age Mass A(Li) Error vsini Hot jupiter Flag Ref.
(K) (cm s-2) (km s-1) (Gyr) (M) (kms-1)

HD  2039 5976 4.45 1.26 0.32 2.03 1.14 2.38 0.06 3.46 no [1] [c]
HD  8574 6151 4.51 1.45 0.06 2.75 1.17 2.65 0.10 no [4] [c]
HD  9826 6212 4.26 1.69 0.13 2.65 1.28 2.87 0.08 yes [4] [c]
HD  11506 6204 4.44 1.32 0.36 0.83 1.23 2.96 0.04 5.01 no [1] [b]
HD  13931 5940 4.42 1.19 0.08 3.15 1.08 1.84 0.15 no [7] [b]
HD  16175 6030 4.23 1.39 0.32 3.22 1.29 2.78 0.07 4.58 no [9] [b]
HD  17156 6084 4.33 1.47 0.23 2.77 1.21 2.84 0.05 no [7] [e]
HD  20367 6138 4.53 1.22 0.17 1.18 1.15 3.00 0.10 no [10] [c]
HD  23596 6108 4.25 1.30 0.31 2.77 1.24 2.83 0.05 no [11] [c]
HD  30562 5970 4.20 1.20 0.32 3.73 1.22 2.78 0.05 no [3] [d]
HD  31253 6147 4.27 1.47 0.17 2.77 1.25 1.75 0.07 3.25 no [3] [b]
HD  33283 6058 4.16 1.41 0.34 2.92 1.34 2.51 0.05 4.08 no [1] [b]
HD  34445 5915 4.30 1.11 0.24 4.36 1.14 1.80 0.08 no [5] [d]
HD  38283 5980 4.27 1.28 –0.14 7.43 1.06 2.43 0.05 3.80 no [3] [b]
HD  40979 6145 4.31 1.29 0.21 0.79 1.19 2.96 0.07 no [4] [c]
HD  43691 6200 4.28 1.49 0.28 2.28 1.28 <2.21 no [7] [i]
HD  50499 6056 4.29 1.23 0.39 2.93 1.20 2.70 0.07 no [5] [d]
HD  50554 6026 4.41 1.11 0.01 1.96 1.09 2.52 0.05 3.93 no [11] [c]
HD  60532 6273 4.02 1.88 –0.09 2.24 1.50 1.90 0.08 5.83 no [2] [b]
HD  68988 5988 4.45 1.25 0.36 1.38 1.14 2.25 0.10 no [4] [c]
HD  74156 6112 4.34 1.38 0.16 2.96 1.25 2.68 0.04 4.31 no [3] [c]
HD  75898 6137 4.31 1.36 0.30 2.54 1.25 2.85 0.06 4.32 no [1] [b]
HD  86081 6036 4.21 1.34 0.22 2.68 1.19 2.00 0.08 4.82 yes [1] [b]
HD  86226 5947 4.54 1.12 0.02 1.05 1.08 2.17 0.06 no [3] [b]
HD  86264 6596 4.47 1.90 0.37 0.81 1.40 <1.15 no [3] [b]
HD  89307 5967 4.51 1.33 –0.13 3.54 1.02 2.31 0.08 no [4] [d]
HD  95128 5954 4.44 1.30 0.06 4.44 1.07 1.85 0.15 no [4] [c]
HD  103774 6732 4.81 2.03 0.29 0.26 1.40 <1.30 7.95 no [2] [b]
HD  118203 5910 4.18 1.34 0.25 3.61 1.29 2.70 0.05 no [4] [b]
HD  120136 6339 4.19 1.70 0.23 1.49 1.30 <1.40 14.20 no [1] [c]
HD  142415 6045 4.53 1.12 0.21 0.51 1.12 2.10 0.10 no [3] [c]
HD  149026 6162 4.37 1.41 0.36 2.34 1.25 2.44 0.10 yes [4] [e]
HD  149143 6018 4.31 1.12 0.45 2.92 1.17 1.95 0.10 yes [5] [d]
HD  150706 5961 4.50 1.11 –0.01 0.56 1.05 2.63 0.04 no [11] [c]
HD  155358 5908 4.26 1.29 –0.62 11.74 0.88 2.14 0.10 3.12 no [1] [b]
HD  164509 5957 4.43 1.09 0.24 0.93 1.13 2.30 0.06 3.60 no [2] [b]
HD  176051 6030 4.68 1.28 –0.04 3.39 1.07 2.54 0.06 no [7] [b]
HD  183263 5991 4.38 1.23 0.34 1.66 1.14 2.36 0.05 no [3] [f]
HD  185269 5983 4.05 1.49 0.10 3.75 1.27 2.49 0.05 no [10] [h]
HD  187085 6146 4.36 1.31 0.13 1.76 1.18 2.66 0.06 3.74 no [1] [b]
HD  196067 5999 4.13 1.30 0.23 3.39 1.23 2.40 0.06 no [3] [b]
HD  196885A 6340 4.46 1.51 0.29 0.52 1.27 2.74 0.05 no [4] [d]
HD  205739 6301 4.40 1.42 0.21 1.74 1.31 2.71 0.04 4.06 no [1] [b]
HD  220689 5904 4.38 1.13 –0.01 4.28 1.03 1.92 0.06 no [3] [b]
HD  220773 5995 4.26 1.33 0.11 4.15 1.21 2.48 0.05 no [3] [b]
HD  224693 6053 4.18 1.40 0.28 3.00 1.32 2.09 0.08 4.20 no [1] [b]
HD  231701 6224 4.37 1.35 0.04 1.35 1.18 2.77 0.04 4.26 no [1] [b]
CoRoT-1 6397 4.66 1.68 0.03 0.95 1.39 2.77 0.06 4.74 no [2] [a]
CoRoT-4 6344 4.82 1.74 0.15 1.20 1.28 <2.43 6.40 no [2] [a]
CoRoT-5 6240 4.46 1.28 0.04 1.83 1.22 2.88 0.07 3.82 yes [2] [a]
HAT-P-1 6076 4.47 1.17 0.21 1.28 1.18 1.77 0.10 yes [4] [e]
HAT-P-4 6054 4.17 1.59 0.35 2.12 1.21 2.90 0.10 yes [7] [e]
HAT-P-6 6855 4.69 2.85 –0.08 0.73 1.24 <1.90 no [7] [e]
HAT-P-7 6525 4.09 1.78 0.31 1.05 1.42 3.29 0.10 no [7] [e]
HAT-P-8 6550 4.80 1.93 0.07 0.53 1.23 3.02 0.10 10.94 no [9] [a]
HAT-P-30 6338 4.52 1.40 0.12 0.85 1.25 3.10 0.06 no [3] [a]
HAT-P-35 6178 4.40 1.34 0.12 1.61 1.21 2.67 0.05 yes [3] [a]
Kepler-21 6409 4.43 1.86 –0.03 2.42 1.36 <1.20 no [7] [j]
Kepler-43 6041 4.26 1.85 0.33 2.34 1.19 2.20 0.15 yes [7] [k]
OGLE-TR-10 6075 4.54 1.45 0.28 2.02 1.22 2.28 0.10 6.43 yes [1] [g]
OGLE-TR-182 5924 4.47 0.91 0.37 2.78 1.16 <1.89 4.53 no [1] [l]
OGLE-TR-211 6325 4.22 1.63 0.11 <1.50 7.10 no [1] [m]
OGLE-TR-56 6119 4.21 1.48 0.25 1.80 1.25 2.63 0.10 5.25 yes [1] [g]
TrES-4 6293 4.20 2.01 0.34 1.36 1.31 <1.50 no [7] [e]
WASP-1 6252 4.32 1.42 0.23 1.17 1.29 3.29 0.08 3.66 yes [1] [a]
WASP-7 6621 4.62 3.00 0.12 0.71 1.22 <1.70 17.48 no [1] [a]
WASP-12 6313 4.37 1.65 0.21 1.18 1.30 2.65 0.08 no [3] [a]
WASP-13 6025 4.19 1.28 0.11 2.93 1.16 2.17 0.08 4.35 yes [8] [a]
WASP-15 6573 4.79 1.72 0.09 0.52 1.30 <2.00 4.77 no [2] [a]
WASP-17 6794 4.83 2.57 –0.12 0.74 1.27 <1.30 8.87 no [2] [a]
WASP-18 6526 4.73 1.83 0.19 0.33 1.28 2.81 0.10 no [3] [a]
WASP-21 5924 4.39 1.06 –0.22 5.29 0.96 2.28 0.10 yes [3] [a]
WASP-22 6153 4.57 1.36 0.26 1.31 1.22 2.49 0.10 4.29 yes [2] [a]
WASP-24 6297 4.76 1.41 0.09 0.84 1.21 2.52 0.08 5.55 yes [2] [a]
WASP-26 6034 4.44 1.28 0.16 1.85 1.16 2.09 0.10 yes [3] [a]
WASP-28 6134 4.55 1.17 –0.12 2.68 1.09 2.51 0.10 4.39 yes [2] [a]
WASP-31 6443 4.76 1.62 –0.08 1.16 1.18 2.97 0.08 6.97 no [2] [a]
WASP-32 6427 4.93 1.20 0.28 0.73 1.20 <1.80 no [3] [a]
WASP-35 6072 4.69 1.26 –0.05 1.82 1.07 2.38 0.08 yes [3] [a]
WASP-36 5928 4.51 0.89 –0.01 3.56 1.05 <1.94 4.01 no [2] [a]
WASP-38 6436 4.80 1.75 0.06 0.35 1.21 <2.20 7.43 no [2] [a]
WASP-54 6296 4.37 1.45 0.00 1.51 1.20 <1.30 no [3] [a]
WASP-55 6070 4.55 1.10 0.09 1.90 1.14 2.51 0.08 yes [3] [a]
WASP-62 6391 4.73 1.50 0.24 0.50 1.26 2.63 0.06 no [3] [a]
WASP-66 7051 5.00 3.07 0.05 0.38 1.45 3.39 0.06 no [3] [a]
WASP-71 6180 4.15 1.69 0.37 1.68 1.27 2.33 0.10 yes [3] [a]
WASP-78 6291 4.19 1.63 –0.07 2.21 1.19 <1.50 no [3] [a]
WASP-79 7002 4.77 2.64 0.19 0.39 1.36 <2.30 no [3] [a]

Notes. The instrument used and the reference for the stellar parameters are shown in the last two columns. Flag: [1] UVES; [2] HARPS; [3] FEROS; [4] SARG; [5] CORALIE; [6] NOT; [7] SOPHIE; [8] HIRES; [9] FIES; [10] ELODIE; [11] UES.

Reference. [a] Mortier et al. (2013); [b] Santos et al. (2013); [c] Santos et al. (2004); [d] Sousa et al. (2006); [e] Ammler-von Eiff et al. (2009); [f] Santos et al. (2005); [g] Santos et al. (2006); [h]Moutou et al. (2006); [i] da Silva et al. (2007); [j] Molenda-Żakowicz et al. (2013); [k] Bonomo et al. (2012); [l] Pont et al. (2008); [m] Udalski et al. (2008).

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