\begin{table}%T4
\caption{Oxygen abundances from [O~I]~line in a set of planet host stars.}\label{longtab4}
\begin{tabular}{lccccccr}
\hline\hline
\noalign{\smallskip}
Star & $T_{\rm eff}$ & $\log {g}$ & $\xi_{\rm t}$ & [Fe/H] & $EW_{[\ion{O}{i}]}$ & [O/H]$_{[\ion{O}{i}]}$ & Instr.\\
 & (K) & (cm~s$^{-2}$) & (km~s$^{-1}$) & & (m\AA) & & \\
\hline 
\object{HD~1237}  & $5536\pm50 $ & $4.56\pm0.12$& $1.33\pm0.06$ & $ 0.12\pm0.06$ & $ 2.9\pm0.5$ & $-0.05\pm0.10$ & [1]\\
\object{HD~23079} & $5959\pm46 $ & $4.35\pm0.12$& $1.20\pm0.10$ & $-0.11\pm0.06$ & $ 3.5\pm0.5$ & $-0.12\pm0.09$ & [1]\\
\object{HD~28185} & $5656\pm44 $ & $4.45\pm0.08$& $1.01\pm0.06$ & $ 0.22\pm0.05$ & $ 5.4\pm0.8$ & $ 0.22\pm0.09$ & [1]\\
\object{HD~30177} & $5591\pm50 $ & $4.35\pm0.12$& $1.03\pm0.06$ & $ 0.39\pm0.06$ & $ 8.3\pm0.5$ & $ 0.44\pm0.07$ & [1]\\
\object{HD~33636 }& $6046\pm49 $ & $4.71\pm0.09$& $1.79\pm0.19$ & $-0.08\pm0.06$ & $ 3.2\pm0.7$ & $ 0.02\pm0.11$ & [1]\\
\object{HD~37124 }& $5546\pm30 $ & $4.50\pm0.03$& $0.80\pm0.07$ & $-0.38\pm0.04$ & $ 4.5\pm0.3$ & $-0.07\pm0.04$ & [1]\\
\object{HD~39091 }& $5991\pm27 $ & $4.42\pm0.10$& $1.24\pm0.04$ & $ 0.10\pm0.04$ & $ 4.9\pm0.5$ & $ 0.13\pm0.07$ & [1]\\
\object{HD~50554 }& $6026\pm30 $ & $4.41\pm0.13$& $1.11\pm0.06$ & $ 0.01\pm0.04$ & $ 4.0\pm0.4$ & $ 0.01\pm0.07$ & [1]\\
\object{HD~65216 }& $5666\pm31 $ & $4.53\pm0.09$& $1.06\pm0.05$ & $-0.12\pm0.04$ & $ 3.7\pm0.5$ & $-0.05\pm0.08$ & [1]\\
\object{HD~72659 }& $5995\pm45 $ & $4.30\pm0.07$& $1.42\pm0.09$ & $ 0.03\pm0.06$ & $ 5.5\pm0.5$ & $ 0.11\pm0.05$ & [1]\\
\object{HD~73256 }& $5518\pm49 $ & $4.42\pm0.12$& $1.22\pm0.06$ & $ 0.26\pm0.06$ & $ 4.8\pm1.0$ & $ 0.17\pm0.12$ & [1]\\
\object{HD~74156 }& $6112\pm39 $ & $4.34\pm0.10$& $1.38\pm0.07$ & $ 0.16\pm0.05$ & $ 4.6\pm0.3$ & $ 0.11\pm0.06$ & [1]\\
\object{HD~106252}& $5899\pm35 $ & $4.34\pm0.07$& $1.08\pm0.06$ & $-0.01\pm0.05$ & $ 4.0\pm0.8$ & $-0.04\pm0.11$ & [1]\\
\object{HD~114729}& $5886\pm36 $ & $4.28\pm0.13$& $1.25\pm0.09$ & $-0.25\pm0.05$ & $ 4.9\pm0.5$ & $-0.06\pm0.07$ & [1]\\
\object{HD~213240}& $5984\pm33 $ & $4.25\pm0.10$& $1.25\pm0.05$ & $ 0.17\pm0.05$ & $ 5.7\pm0.4$ & $ 0.15\pm0.06$ & [1]\\
\object{HD~216435}& $5938\pm42 $ & $4.12\pm0.05$& $1.28\pm0.06$ & $ 0.24\pm0.05$ & $ 6.7\pm0.7$ & $ 0.18\pm0.06$ & [1]\\
\object{HD~216437}& $5887\pm32 $ & $4.30\pm0.07$& $1.31\pm0.04$ & $ 0.25\pm0.04$ & $ 6.2\pm0.5$ & $ 0.23\pm0.05$ & [1]\\
\object{BD~103166}&$ 5325\pm45  $&$ 4.36\pm0.07 $&$ 0.95\pm0.05 $&$  0.35\pm0.05$ &$ 3.9\pm1.0 $&$ 0.06\pm0.13$&[3]\\
\object{HD~2039}  & $5976\pm51 $ & $4.45\pm0.10$ & $1.26\pm0.07$ &$ 0.32\pm0.06 $&$ 4.2\pm1.0  $&$ 0.14\pm0.12$&[5]\\
\object{HD~3651}  & $5173\pm35 $ & $4.37\pm0.12$ & $0.74\pm0.05$ &$ 0.12\pm0.04 $&$ 5.1\pm0.5  $&$ 0.12\pm0.08$&[4]\\
\object{HD~4203}  & $5636\pm40 $ & $4.23\pm0.14$ & $1.12\pm0.05$ &$ 0.40\pm0.05 $&$ 3.8\pm1.5  $&$ 0.00\pm0.21$&[3]\\
\object{HD~9826}  & $6212\pm64 $ & $4.26\pm0.13$ & $1.69\pm0.16$ &$ 0.13\pm0.08 $&$ 4.0\pm0.7  $&$ 0.02\pm0.10$&[2]\\
\object{HD~16141} & $5801\pm30 $ & $4.22\pm0.12$ & $1.34\pm0.04$ &$ 0.15\pm0.04 $&$4.7\pm1.0   $&$ 0.01\pm0.11$&[3]\\
\object{HD~17051} & $6252\pm53 $ & $4.61\pm0.16$ & $1.18\pm0.10$ &$ 0.26\pm0.06 $&$ 3.6\pm0.7  $&$ 0.16\pm0.11$&[1]\\
\object{HD~19994} & $6190\pm00 $ & $4.19\pm0.00$ & $1.54\pm0.00$ &$ 0.24\pm0.00 $&$ 5.0\pm1.0  $&$ 0.11\pm0.09$&[1]\\
\object{HD~22049} & $5073\pm42 $ & $4.43\pm0.08$ & $1.05\pm0.06$ &$-0.13\pm0.05 $&$ 3.8\pm0.8  $&$-0.07\pm0.10$&[2]\\
\object{HD~23079} & $5959\pm46 $ & $4.35\pm0.12$ & $1.20\pm0.10$ &$-0.11\pm0.06 $&$ 4.2\pm0.2  $&$-0.04\pm0.06$&[3]\\
\object{HD~23596} & $6108\pm36 $ & $4.25\pm0.10$ & $1.30\pm0.05$ &$ 0.31\pm0.05 $&$ 5.4\pm0.3  $&$ 0.18\pm0.05$&[2]\\
\object{HD~27442} & $4825\pm107$ & $3.55\pm0.32$ & $1.18\pm0.12$ &$ 0.39\pm0.13 $&$15.6\pm1.5  $&$ 0.36\pm0.16$&[3]\\
\object{HD~28185} & $5656\pm44 $ & $4.45\pm0.08$ & $1.01\pm0.06$ &$ 0.22\pm0.05 $&$ 3.6\pm1.0  $&$ 0.02\pm0.15$&[5]\\
\object{HD~30177} & $5587\pm00 $ & $4.29\pm0.00$ & $1.08\pm0.00$ &$ 0.38\pm0.00 $&$ 3.3\pm1.0  $&$-0.04\pm0.15$&[5]\\
\object{HD~38529} & $5674\pm40 $ & $3.94\pm0.12$ & $1.38\pm0.05$ &$ 0.40\pm0.06 $&$13.3\pm0.7  $&$ 0.44\pm0.06$&[3]\\
\object{HD~46375} & $5268\pm55 $ & $4.41\pm0.16$ & $0.97\pm0.06$ &$ 0.20\pm0.06 $&$ 5.9\pm0.5  $&$ 0.23\pm0.09$&[2]\\
\object{HD~50554} & $6026\pm30 $ & $4.41\pm0.13$ & $1.11\pm0.06$ &$ 0.01\pm0.04 $&$ 5.3\pm0.9  $&$ 0.14\pm0.09$&[2]\\
\object{HD~52265} & $6105\pm00 $ & $4.28\pm0.00$ & $1.36\pm0.00$ &$ 0.23\pm0.00 $&$ 5.1\pm0.7  $&$ 0.14\pm0.05$&[3]\\
\object{HD~59686 }& $4871\pm135$ & $3.15\pm0.24$ & $1.85\pm0.12$ &$  0.28\pm0.18$ &$33.8\pm1.0 $&$ 0.52\pm0.13$&[3]\\
\object{HD~70642 }&$ 5671\pm46  $&$ 4.39\pm0.05 $&$ 1.01\pm0.06 $&$  0.20\pm0.06$ &$ 5.5\pm0.5 $&$ 0.17\pm0.05$&[3]\\
\object{HD~73256} & $5518\pm49 $ & $4.42\pm0.12$ & $1.22\pm0.06$ &$ 0.26\pm0.06 $&$ 3.5\pm0.9  $&$ 0.01\pm0.14$&[3]\\
\object{HD~74156} & $6112\pm39 $ & $4.34\pm0.10$ & $1.38\pm0.07$ &$ 0.16\pm0.05 $&$ 7.3\pm0.7  $&$ 0.31\pm0.06$& [3]\\
\object{HD~75289} & $6143\pm53 $ & $4.42\pm0.13$ & $1.53\pm0.09$ &$ 0.28\pm0.07 $&$ 5.6\pm0.4  $&$ 0.14\pm0.08$& [1]\\
\object{HD~75732} & $5279\pm62 $ & $4.37\pm0.18$ & $0.98\pm0.07$ &$ 0.33\pm0.07 $&$ 4.5\pm0.7  $&$ 0.13\pm0.11$& [2]\\
\object{HD~82943} & $6015\pm00 $ & $4.46\pm0.00$ & $1.13\pm0.00$ &$ 0.30\pm0.00 $&$ 4.8\pm0.7  $&$ 0.20\pm0.06$& [1]\\
\object{HD~83443 }&$ 5501\pm63  $&$ 4.46\pm0.09 $&$ 1.07\pm0.08 $&$  0.39\pm0.07$ &$ 4.4\pm1.0 $&$ 0.17\pm0.13$&[3]\\
\object{HD~92788 }&$ 5758\pm37  $&$ 4.3 \pm0.04 $&$ 1.1 \pm0.04 $&$  0.34\pm0.05$ &$ 3.8\pm1.0 $&$ 0.02\pm0.13$&[3]\\
\object{HD~95128} & $5954\pm25 $ & $4.44\pm0.10$ & $1.30\pm0.04$ &$ 0.06\pm0.03 $&$ 5.2\pm0.6  $&$ 0.15\pm0.06$&[4]\\
\object{HD~106252}&$ 5834\pm37  $&$ 4.22\pm0.02 $&$ 1.06\pm0.06 $&$ -0.03\pm0.05$ &$ 7.0\pm1.0 $&$ 0.14\pm0.07$&[3]\\
\object{HD~108147}& $6248\pm42 $ & $4.49\pm0.16$ & $1.35\pm0.08$ &$ 0.20\pm0.05 $&$ 3.7\pm0.4  $&$ 0.11\pm0.09$&[1]\\
\object{HD~108874}& $5596\pm42 $ & $4.37\pm0.12$ & $0.89\pm0.05$ &$ 0.23\pm0.05 $&$ 3.0\pm0.7  $&$-0.10\pm0.12$&[2]\\
\object{HD~114386}&$ 4865\pm93  $&$ 4.3 \pm0.17 $&$ 0.86\pm0.12 $&$ -0.04\pm0.07$ &$ 5.1\pm1.0 $&$ 0.07\pm0.15$&[3]\\
\object{HD~114762}& $5884\pm34 $ & $4.22\pm0.02$ & $1.31\pm0.17$ &$-0.70\pm0.04 $&$ 3.2\pm0.1  $&$-0.36\pm0.02$&[1]\\
\object{HD~114783}& $5098\pm36 $ & $4.45\pm0.11$ & $0.74\pm0.05$ &$ 0.09\pm0.04 $&$ 4.4\pm1.5  $&$ 0.08\pm0.18$&[4]\\
\object{HD~117176}& $5560\pm34 $ & $4.07\pm0.05$ & $1.18\pm0.05$ &$-0.06\pm0.05 $&$ 7.1\pm0.5  $&$ 0.05\pm0.04$&[4]\\
\object{HD~121504}& $6075\pm40 $ & $4.64\pm0.12$ & $1.31\pm0.07$ &$ 0.16\pm0.05 $&$ 3.5\pm0.2  $&$ 0.10\pm0.06$&[1]\\
\object{HD~128311}& $4835\pm72 $ & $4.44\pm0.21$ & $0.89\pm0.11$ &$ 0.03\pm0.07 $&$ 6.0\pm1.5  $&$ 0.19\pm0.16$&[2]\\
\object{HD~134987}& $5776\pm29$ & $4.36\pm0.07$ & $1.09\pm0.04$ &$ 0.30\pm0.04 $&$ 6.5\pm0.5   $&$ 0.27\pm0.05$&[4]\\
\object{HD~137759}& $4775\pm113$& $3.09\pm0.40$ & $1.78\pm0.11$ &$ 0.13\pm0.14 $&$34.7\pm1.0   $&$ 0.48\pm0.19$&[4]\\
\object{HD~141937}& $5909\pm39$ & $4.51\pm0.08$ & $1.13\pm0.06$ &$ 0.10\pm0.05 $&$ 4.6\pm0.7   $&$ 0.13\pm0.07$&[2]\\
\object{HD~143761}& $5853\pm25$ & $4.41\pm0.15$ & $1.35\pm0.07$ &$-0.21\pm0.04 $&$ 4.5\pm0.8   $&$-0.02\pm0.11$&[4]\\
\object{HD~145675}& $5311\pm87$ & $4.42\pm0.18$ & $0.92\pm0.10$ &$ 0.43\pm0.08 $&$ 5.7\pm1.0   $&$ 0.29\pm0.12$&[4]\\
\object{HD~147513}&$ 5894\pm31  $&$ 4.43\pm0.02 $&$ 1.26\pm0.05 $&$  0.08\pm0.04$ &$ 5.0\pm1.5 $&$ 0.12\pm0.16$&[3]\\
\object{HD~150706}& $5961\pm27$ & $4.50\pm0.10$ & $1.11\pm0.06$ &$-0.01\pm0.04 $&$ 2.8\pm0.5   $&$-0.12\pm0.09$&[2]\\
\object{HD~168443}& $5617\pm35$ & $4.22\pm0.05$ & $1.21\pm0.05$ &$ 0.06\pm0.05 $&$ 6.3\pm1.0   $&$ 0.11\pm0.08$&[4]\\
\object{HD~168746}& $5601\pm33$ & $4.41\pm0.12$ & $0.99\pm0.05$ &$-0.08\pm0.05 $&$ 6.8\pm0.5   $&$ 0.19\pm0.07$&[4]\\
\object{HD~177830}& $4804\pm77$ & $3.57\pm0.17$ & $1.14\pm0.09$ &$ 0.33\pm0.09 $&$16.0\pm0.7   $&$ 0.38\pm0.09$&[4]\\
\object{HD~178911B}&$5600\pm42$ & $4.44\pm0.08$ & $0.95\pm0.05$ &$ 0.27\pm0.05 $&$ 5.9\pm1.0   $&$ 0.25\pm0.08$&[4]\\
\object{HD~179949}& $6260\pm43$ & $4.43\pm0.05$ & $1.41\pm0.09$ &$ 0.22\pm0.05 $&$ 2.9\pm1.0   $&$-0.02\pm0.18$&[4]\\
\object{HD~186427}& $5772\pm25$ & $4.40\pm0.07$ & $1.07\pm0.04$ &$ 0.08\pm0.04 $&$ 3.0\pm0.3   $&$-0.13\pm0.05$&[4]\\
\object{HD~187123}& $5845\pm22$ & $4.42\pm0.07$ & $1.10\pm0.03$ &$ 0.13\pm0.03 $&$ 5.6\pm0.5   $&$ 0.18\pm0.05$&[4]\\
\object{HD~190360}& $5584\pm36$ & $4.37\pm0.06$ & $1.07\pm0.05$ &$ 0.24\pm0.05 $&$ 6.1\pm0.6   $&$ 0.22\pm0.04$&[2]\\
\object{HD~192263}& $4947\pm58$ & $4.51\pm0.20$ & $0.86\pm0.09$ &$-0.02\pm0.06 $&$ 4.1\pm1.0   $&$ 0.04\pm0.15$&[3]\\
\object{HD~195019}& $5842\pm31$ & $4.32\pm0.07$ & $1.27\pm0.05$ &$ 0.09\pm0.04 $&$ 3.7\pm0.7   $&$-0.07\pm0.09$&[2]\\
\object{HD~209458}& $6117\pm26$ & $4.48\pm0.08$ & $1.40\pm0.06$ &$ 0.02\pm0.03 $&$ 4.0\pm0.8   $&$ 0.06\pm0.10$&[1]\\
\object{HD~210277}& $5532\pm00$ & $4.29\pm0.00$ & $1.03\pm0.00$ &$ 0.19\pm0.00 $&$ 6.6\pm0.5   $&$ 0.21\pm0.04$&[4]\\
\object{HD~213240}& $5984\pm33$ & $4.25\pm0.10$ & $1.25\pm0.05$ &$ 0.17\pm0.05 $&$ 9.0\pm1.5   $&$ 0.35\pm0.09$&[5]\\
\object{HD~216770}& $5423\pm41$ & $4.40\pm0.13$ & $1.01\pm0.05$ &$ 0.26\pm0.04 $&$10.2\pm2.0   $&$ 0.49\pm0.12$&[4]\\
\object{HD~217014}& $5804\pm36$ & $4.42\pm0.07$ & $1.20\pm0.05$ &$ 0.20\pm0.05 $&$ 5.4\pm1.0   $&$ 0.19\pm0.11$&[3]\\
\object{HD~217107}& $5645\pm00$ & $4.31\pm0.00$ & $1.06\pm0.00$ &$ 0.37\pm0.00 $&$ 5.4\pm0.2   $&$ 0.18\pm0.01$&[2]\\
\object{HD~222582}& $5843\pm38$ & $4.45\pm0.07$ & $1.03\pm0.06$ &$ 0.05\pm0.05 $&$ 4.8\pm1.0   $&$ 0.10\pm0.11$&[2]\\
\object{HD~104985}& $4773\pm62 $ & $2.76\pm0.14$ & $1.71\pm0.07$ &$-0.28\pm0.09 $ &$42.7\pm1.5 $&$ 0.30\pm0.07^1$&[4]\\
\hline
\end{tabular}
The instruments used to obtain the spectra were: [1] UVES; [2] UES; [3] FEROS; [4] SARG; [5] CORALIE.\\
$^1$ This value was excluded from the figures since it is inconsistent with the triplet result.
\end{table}