\begin{table}%t1
\caption{Planet-host stars studied in this paper. See text for more details.}\label{tab:planets}
%\centerline
{
\begin{tabular}{lcccrccccc}
\hline
\hline
HD     & $T_{{\rm eff}}$ & $\log{g}_{{\rm spec}}$ & $\xi_{{\rm t}}$ & \multicolumn{1}{c}{[Fe/H]} & $N$(\ion{Fe}{i}, \ion{Fe}{ii}) & $\sigma$(\ion{Fe}{i}, \ion{Fe}{ii}) & Instr.$\dagger$ & Mass         & $\log{g}_{{\rm hipp}}$ \\
number & [K]                &  [cm~s$^{-2}$]  &  [km~s$^{-1}$]  &        &                              &                                    &            & [$M_{\odot}$] & [cm~s$^{-2}$] \\
\hline
\object{BD$-$10~3166} & 5325 $\pm$ 45  & 4.36 $\pm$ 0.21 & 0.95 $\pm$ 0.05 & 0.35 $\pm$ 0.05 & 35, 9  & 0.05, 0.10 & [a]  &  --  &   --\\
\object{HD~2638}   & 5192 $\pm$ 38  & 4.29 $\pm$ 0.25 & 0.86 $\pm$ 0.04 & 0.16 $\pm$ 0.04    & 35, 6  & 0.04, 0.12 & [g]  & 0.82 & 4.50\\
\object{HD~27894}  & 4875 $\pm$ 81  & 4.22 $\pm$ 0.26 & 0.65 $\pm$ 0.14 & 0.30 $\pm$ 0.07    & 35, 5  & 0.07, 0.10 & [g]  & 0.68	& 4.43\\
\object{HD~37605}  & 5391 $\pm$ 49  & 4.37 $\pm$ 0.18 & 0.97 $\pm$ 0.06 & 0.31 $\pm$ 0.06    & 38, 6  & 0.05, 0.08 & [a]  & 0.95 & 4.54\\
\object{HD~41004~A}  & 5242 $\pm$ 57  & 4.35 $\pm$ 0.22 & 1.01 $\pm$ 0.07 & 0.16 $\pm$ 0.07 & 39, 6  & 0.06, 0.10 & [a]  & 0.80 & 4.39\\
\object{HD~59686}  & 4871 $\pm$ 135 & 3.15 $\pm$ 0.41 & 1.85 $\pm$ 0.12 & 0.28 $\pm$ 0.18    & 39, 10 & 0.16, 0.18 & [a]  & --   &   --\\
\object{HD~63454}  & 4841 $\pm$ 65  & 4.23 $\pm$ 0.30 & 0.89 $\pm$ 0.09 & 0.11 $\pm$ 0.07    & 35, 5  & 0.06, 0.15 & [g]  & 0.69 & 4.57\\
\object{HD~70642}  & 5671 $\pm$ 46  & 4.39 $\pm$ 0.27 & 1.01 $\pm$ 0.06 & 0.20 $\pm$ 0.06    & 39, 12 & 0.05, 0.11 & [a]  & 0.98 & 4.42\\
\object{HD~70642}  & 5693 $\pm$ 26  & 4.41 $\pm$ 0.09 & 1.01 $\pm$ 0.04 & 0.18 $\pm$ 0.04    & 36, 8  & 0.03, 0.04 & [c]  & 0.99 & 4.43\\
\object{HD~70642}  & 5682         & 4.40          & 1.01          & 0.19             & --    & --        & avg. & 0.98 & 4.42\\
\object{HD~83443}  & 5501 $\pm$ 63  & 4.46 $\pm$ 0.36 & 1.07 $\pm$ 0.08 & 0.39 $\pm$ 0.07    & 39, 11 & 0.07, 0.16 & [a]  & 0.96 & 4.41\\
\object{HD~83443}  & 5454 $\pm$ 61  & 4.33 $\pm$ 0.17 & 1.08 $\pm$ 0.08 & 0.35 $\pm$ 0.08    & 38, 7  & 0.07, 0.08 & [c]  & 0.93 & 4.37\\
\object{HD~83443}  & 5478         & 4.40          & 1.08          & 0.37             & --    & --        & avg. & 0.94 & 4.39\\
\object{HD~88133}  & 5438 $\pm$ 34  & 3.94 $\pm$ 0.11 & 1.16 $\pm$ 0.03 & 0.33 $\pm$ 0.05    & 35, 7  & 0.04, 0.04 & [d]  & 0.98 & 3.83\\
\object{HD~92788}  & 5758 $\pm$ 37  & 4.30 $\pm$ 0.16 & 1.10 $\pm$ 0.04 & 0.34 $\pm$ 0.05    & 38, 11 & 0.04, 0.07 & [a]  & 1.06 & 4.44\\
\object{HD~92788}  & 5821 $\pm$ 41  & 4.45 $\pm$ 0.06 & 1.16 $\pm$ 0.05 & 0.32 $\pm$ 0.05    & 37, 5  & 0.04, 0.02 & [c]  & 1.12 & 4.49\\
\object{HD~92788}  & 5790         & 4.38          & 1.13          & 0.33             & --    & --        & avg. & 1.09 & 4.46\\
\object{HD~93083}  & 4995 $\pm$ 50  & 4.26 $\pm$ 0.19 & 0.66 $\pm$ 0.08 & 0.15 $\pm$ 0.06    & 36, 5  & 0.05, 0.08 & [h]  & 0.70 & 4.43\\
\object{HD~99492}  & 4810 $\pm$ 72  & 4.21 $\pm$ 0.21 & 0.72 $\pm$ 0.13 & 0.26 $\pm$ 0.07    & 33, 4  & 0.07, 0.09 & [d]  & --   & --\\
\object{HD~101930} & 5079 $\pm$ 62  & 4.24 $\pm$ 0.16 & 0.73 $\pm$ 0.08 & 0.17 $\pm$ 0.06    & 36, 5  & 0.05, 0.06 & [h]  & 0.74	& 4.40\\
\object{HD~102117} & 5708 $\pm$ 46  & 4.34 $\pm$ 0.10 & 1.15 $\pm$ 0.06 & 0.33 $\pm$ 0.06    & 39, 8  & 0.05, 0.03 & [a]  & 1.05 & 4.25\\
\object{HD~102117} & 5672 $\pm$ 22  & 4.27 $\pm$ 0.07 & 1.05 $\pm$ 0.02 & 0.30 $\pm$ 0.03    & 37, 8  & 0.03, 0.03 & [h]  & 1.03 & 4.23\\
\object{HD~102117} & 5690         & 4.30          & 1.10          & 0.32             & --    & --        & avg. & 1.04	& 4.24\\
\object{HD~104985} & 4773 $\pm$ 62  & 2.76 $\pm$ 0.14 & 1.71 $\pm$ 0.07 & $-$0.28 $\pm$ 0.09 & 33, 9  & 0.09, 0.05 & [b]  &  --  &   --\\
\object{HD~106252} & 5834 $\pm$ 37  & 4.22 $\pm$ 0.12 & 1.06 $\pm$ 0.06 & $-$0.03 $\pm$ 0.05 & 39, 11 & 0.04, 0.06 & [a]  & 0.98 & 4.35\\
\object{HD~106252} & 5899 $\pm$ 35  & 4.34 $\pm$ 0.07 & 1.08 $\pm$ 0.06 & $-$0.01 $\pm$ 0.05 & 37, 6  & 0.04, 0.04 & [c]  & 1.02 & 4.39\\
\object{HD~106252} & 5866         & 4.28          & 1.07          & $-$0.02          & --	 & --        & avg. & 1.00 & 4.37\\
\object{HD~114386} & 4865 $\pm$ 93  & 4.30 $\pm$ 0.30 & 0.86 $\pm$ 0.12 & $-$0.04 $\pm$ 0.07 & 37, 8  & 0.06, 0.13 & [a]  & 0.66 & 4.52\\
\object{HD~114386} & 4804 $\pm$ 61  & 4.36 $\pm$ 0.28 & 0.57 $\pm$ 0.12 & $-$0.08 $\pm$ 0.06 & 35, 4  & 0.06, 0.14 & [c]  & 0.54 & 4.40\\
\object{HD~114386} & 4834         & 4.33          & 0.72          & $-$0.06          & --	 & --        & avg. & 0.60 & 4.46\\
\object{HD~117207} & 5654 $\pm$ 33 & 4.32 $\pm$ 0.05 & 1.13 $\pm$ 0.04 & 0.23 $\pm$ 0.05     & 37, 7  & 0.04, 0.02 & [d]  & 0.99  & 4.33\\
\object{HD~117618} & 6013 $\pm$ 41 & 4.39 $\pm$ 0.07 & 1.73 $\pm$ 0.09 & 0.06 $\pm$ 0.06     & 37, 7  & 0.05, 0.03 & [d]  & 1.10  & 4.35\\
\object{HD~142022~A} & 5499 $\pm$ 27 & 4.36 $\pm$ 0.04 & 0.94 $\pm$ 0.03 & 0.19 $\pm$ 0.04  & 36, 6  & 0.03, 0.03 & [i]  & 0.90  & 4.33\\
\object{HD~147513}  & 5894 $\pm$ 31   & 4.43 $\pm$ 0.17 & 1.26 $\pm$ 0.05 &  0.08 $\pm$ 0.04 & 39, 11  & 0.04, 0.07 & [a] & 1.13  & 4.54\\
\object{HD~147513}  & 5883 $\pm$ 25   & 4.51 $\pm$ 0.05 & 1.18 $\pm$ 0.04 &  0.06 $\pm$ 0.04 & 36, 7   & 0.03, 0.03 & [c] & 1.11  & 4.53\\
\object{HD~147513}  & 5888          & 4.47          & 1.22          &  0.07          & --     & --        & avg.& 1.12  & 4.54\\
\object{HD~154857} & 5610 $\pm$ 27  & 4.02 $\pm$ 0.12 & 1.30 $\pm$ 0.05 & $-$0.23 $\pm$ 0.04 & 38, 8  & 0.03, 0.05 & [a]  & 1.29 & 3.79\\
\object{HD~160691} & 5813 $\pm$ 42  & 4.25 $\pm$ 0.07 & 1.30 $\pm$ 0.05 & 0.32 $\pm$ 0.05    & 37, 8  & 0.04, 0.03 & [e]  & 1.10 & 4.25\\
\object{HD~160691} & 5798 $\pm$ 33  & 4.31 $\pm$ 0.08 & 1.19 $\pm$ 0.04 & 0.32 $\pm$ 0.04    & 36, 7  & 0.04, 0.03 & [c]  & 1.10 & 4.25\\
\object{HD~160691} & 5806         & 4.28          & 1.24          & 0.32             & --    & --        & avg. & 1.10 & 4.25\\
\object{HD~183263} & 5991 $\pm$ 28  & 4.38 $\pm$ 0.17 & 1.23 $\pm$ 0.04 & 0.34 $\pm$ 0.04    & 38, 8  & 0.03, 0.07 & [a]  & 1.18 & 4.36\\
\object{HD~188015} & 5793 $\pm$ 39  & 4.49 $\pm$ 0.10 & 1.14 $\pm$ 0.05 & 0.30 $\pm$ 0.05    & 38, 7  & 0.04, 0.04 & [a]  & 1.08 & 4.41\\
\object{HD~208487} & 6141 $\pm$ 29  & 4.52 $\pm$ 0.15 & 1.54 $\pm$ 0.07 & 0.06 $\pm$ 0.04    & 38, 8  & 0.03, 0.06 & [a]  & 1.17 & 4.41\\
\object{HD~219449} & 4757 $\pm$ 102 & 2.71 $\pm$ 0.25 & 1.71 $\pm$ 0.09 & 0.05 $\pm$ 0.14    & 31, 8  & 0.12, 0.09 & [b]  &  --  &   --\\
\object{HD~330075} & 5017 $\pm$ 53  & 4.22 $\pm$ 0.11 & 0.69 $\pm$ 0.08 & 0.08 $\pm$ 0.06    & 35, 5  & 0.05, 0.20 & [f]  & 0.69 & 4.37\\
\hline
\end{tabular}}
\medskip
$\dagger$ The instruments used to obtain the spectra were: [a] 2.2-m ESO/FEROS; [b] TNG/SARG; [c] From Paper~IV
\citep[][]{Santos-2004b}; [d] VLT Kueyen/UVES; [e]--[i] HARPS -- From \citet[][]{Santos-2004a}, \citet[][]{Pepe-2004}, 
\citet[][]{Moutou-2005}, \citet[][]{Lovis-2005} and \citet[][]{Eggenberger-2005}, respectively (stellar parameters and~[Fe/H] derived by our team).
\end{table}