\begin{table}%T1
\par
\caption{\label{tab1}Determined atmospheric parameters and Li abundances for a set of stars
with planets and brown dwarf companions.}
%\centering
\par
\begin{tabular}{lccccl}
\hline\hline
\noalign{\smallskip}
Star & $T_{\rm eff}$ & $\log{g}$       & $\xi_t$    & [Fe/H]  & $\log \epsilon({\rm Li}$) \\
     & (K)              &  (cm~s$^{-2}$) & (km~s$^{-1}$) &       &   \\
\noalign{\smallskip}\hline
\noalign{\smallskip}
\object{HD~142 }   & 6290 & 4.38 & 1.91   & 0.11     & 2.96        \\
\object{HD~1237  } & 5555 & 4.65 & 1.50   & 0.11     & 2.24        \\
\object{HD~2039  } & 5990 & 4.56 & 1.23   & 0.34     & 2.29       \\
\object{HD~4203  } & 5650 & 4.38 & 1.15   & 0.40     & $<$0.70      \\
\object{HD~4208  } & 5625 & 4.54 & 0.95   & $-$0.23  & $<$0.69      \\
\object{HD~6434  } & 5790 & 4.56 & 1.40   & $-$0.55  & $<$0.85      \\
\object{HD~8574  } & 6080 & 4.41 & 1.25   & 0.05     & 2.71        \\
\object{HD~9826  } & 6120 & 4.07 & 1.50   & 0.10     & 2.47        \\
\object{HD~10697 } & 5665 & 4.18 & 1.19   & 0.14     & 1.98      \\
\object{HD~12661 } & 5715 & 4.49 & 1.09   & 0.36     & $<$0.99    \\
\object{HD~13445 } & 5190 & 4.71 & 0.78   & $-$0.20  & $<$$-0.1$    \\
\object{HD~16141 } & 5805 & 4.28 & 1.37   & 0.15     & 1.11       \\
\object{HD~17051 } & 6225 & 4.65 & 1.20   & 0.25     & 2.63       \\
\object{HD~19994 } & 6210 & 4.20 & 1.52   & 0.26     & 2.01       \\
\object{HD~20367 } & 6100 & 4.55 & 1.31   & 0.14     & 3.02       \\
\object{HD~22049 } & 5135 & 4.70 & 1.14   & $-$0.07  & $<$0.3    \\
\object{HD~23079 } & 5945 & 4.44 & 1.21   & $-$0.11  & 2.37       \\
\object{HD~23596 } & 6125 & 4.29 & 1.32   & 0.32     & 2.93       \\
\object{HD~27442 } & 4890 & 3.89 & 1.24   & 0.42     & $<$$-0.42$ \\
\object{HD~28185 } & 5705 & 4.59 & 1.09   & 0.24     &  1.55    \\
\object{HD~30177 } & 5590 & 4.45 & 1.07   & 0.39     & $<$0.35   \\
\object{HD~33636 } & 5990 & 4.68 & 1.22   & $-$0.05  & 2.60      \\
\object{HD~37124 } & 5565 & 4.62 & 0.90   & $-$0.37  & $<$0.32   \\
\object{HD~38529 } & 5675 & 4.01 & 1.39   & 0.39     & $<$0.61  \\
\object{HD~39091 } & 5995 & 4.48 & 1.30   & 0.09     & 2.33      \\
\object{HD~46375 } & 5315 & 4.54 & 1.11   & 0.21     & $<$0.02  \\
\object{HD~50554 } & 6050 & 4.59 & 1.19   & 0.02     & 2.59     \\
\object{HD~52265 } & 6100 & 4.29 & 1.31   & 0.24     & 2.88      \\
\object{HD~74156 } & 6105 & 4.40 & 1.36   & 0.15     & 2.74      \\
\object{HD~75289 } & 6135 & 4.43 & 1.50   & 0.27     & 2.84     \\
\object{HD~75732}  & 5307 & 4.58 & 1.06   & 0.35    & $<$0.02   \\
\object{HD~80606}  & 5570 & 4.56 & 1.11   & 0.34     & $<$0.62  \\
\object{HD~82943}  & 6025 & 4.54 & 1.10   & 0.33     & 2.52      \\
\object{HD~83443}  & 5500 & 4.50 & 1.12   & 0.39     & $<$0.56  \\
\object{HD~89744}  & 6338 & 4.17 & 1.55   & 0.30     & 2.07      \\
\object{HD~92788}  & 5820 & 4.60 & 1.11   & 0.34     & 1.34      \\
\object{HD~95128}  & 5925 & 4.45 & 1.24   & 0.00     & 1.8       \\
\object{HD~106252} & 5890 & 4.40 & 1.06   & $-$0.01  & 1.65     \\
\object{HD~108147} & 6265 & 4.59 & 1.40   & 0.20     & 2.34     \\
\object{HD~108874} & 5615 & 4.58 & 0.93   & 0.25     & $<$0.37   \\
\object{HD~114386} & 4875 & 4.69 & 0.63   & 0.00     & $<$$ -0.47$  \\
\object{HD~114729} & 5820 & 4.20 & 1.03   & $-$0.26  & 1.96       \\
\object{HD~114762} & 5950 & 4.45 & 1.0    & $-$0.60  & 2.26      \\
\object{HD~114783} & 5160 & 4.75 & 0.78   & 0.16     & $-$0.12    \\
\object{HD~117176} & 5530 & 4.05 & 1.08   &$-$0.05   & 1.85      \\
\object{HD~121504} & 6090 & 4.73 & 1.35   & 0.17     & 2.66       \\
\object{HD~128311} & 4950 & 4.80 & 1.00   & 0.10     & $< $$-0.37$  \\
\object{HD~130322} & 5430 & 4.62 & 0.92   & 0.06     & $<$0.16   \\
\object{HD~134987} & 5780 & 4.45 & 1.06   & 0.32     & $<$0.74    \\
\object{HD~136118} & 6175 & 4.18 & 1.61   & $-$0.06  & 2.40      \\
\object{HD~141937} & 5925 & 4.62 & 1.16   & 0.11     & 2.48      \\
\object{HD~143761} & 5750 & 4.10 & 1.2    &$-$0.29   & 1.38      \\
\object{HD~145675} & 5255 & 4.40 & 0.68   & 0.51     & $<$$ -0.02$  \\
\object{HD~147513} & 5880 & 4.58 & 1.17   & 0.07     & 2.05       \\
\object{HD~150706} & 6000 & 4.62 & 1.16   & 0.01     & 2.75      \\
\object{HD~160691} & 5820 & 4.44 & 1.23   & 0.33     & $<$0.86   \\
\object{HD~162020} & 4830 & 4.76 & 0.72   & 0.01     & $<$$-0.3$   \\
\object{HD~168443} & 5600 & 4.30 & 1.18   & 0.10     & $<$0.76   \\
\object{HD~168746} & 5610 & 4.50 & 1.02   &$-$0.06   & $<$0.85    \\
\object{HD~169830} & 6300 & 4.04 & 1.37   & 0.22     & 1.16       \\
\object{HD~177830} & 4840 & 3.60 & 1.18   & 0.32     & $<$$ -0.50$ \\
\object{HD~178911B} & 5650 & 4.65 & 0.85   & 0.28    & $<$0.39   \\
\object{HD~179949} & 6235 & 4.41 & 1.38   & 0.21     & 2.63      \\
\object{HD~186427} & 5685 & 4.26 & 0.80   & 0.07     & $<$0.60   \\
\object{HD~187123} & 5830 & 4.40 & 1.00   & 0.16     & 1.20    \\
\object{HD~190228} & 5325 & 3.95 & 1.10   &$-$0.23   & 1.23      \\
\object{HD~190360} & 5590 & 4.48 & 1.06   & 0.25     & $<$0.34    \\
\object{HD~192263} & 4995 & 4.76 & 0.90   & 0.04     & $<$$ -0.35$  \\
\object{HD~195019} & 5845 & 4.39 & 1.23   & 0.08     & 1.46      \\
\object{HD~196050} & 5905 & 4.41 & 1.40   & 0.21     & 2.15      \\
\object{HD~202206} & 5765 & 4.75 & 0.99   & 0.37     & 1.05     \\
\object{HD~209458} & 6120 & 4.56 & 1.37   & 0.03     &  2.70    \\
\object{HD~210277} & 5560 & 4.46 & 1.03   & 0.21     & $<$0.32    \\
\object{HD~213240} & 5975 & 4.32 & 1.30   & 0.16     & 2.56     \\
\object{HD~216435} & 5905 & 4.16 & 1.26   & 0.22     & 2.72      \\
\object{HD~216437} & 5875 & 4.38 & 1.30   & 0.25     & 1.95      \\
\object{HD~217014} & 5805 & 4.51 & 1.22   & 0.21     & 1.30      \\
\object{HD~217107} & 5655 & 4.42 & 1.11   & 0.38     & $<$0.41  \\
\object{HD~222582} & 5850 & 4.58 & 1.06   & 0.06     & $<$0.59   \\
\hline
\end{tabular} 
\end{table}