\begin{table}%t5
\caption{Oxygen abundances from [O~I]~line in a set of comparison stars.}
\label{longtab5}
\begin{tabular}{lccccccr}
\hline\hline
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~1581}  & $5956\pm44$ & $4.39\pm0.13$ & $1.07\pm0.09 $&$-0.14\pm0.05 $&$ 4.8\pm0.2   $&$ 0.03\pm0.07$& [3]\\
\object{HD~7570}  & $6140\pm41$ & $4.39\pm0.16$ & $1.50\pm0.08 $&$ 0.18\pm0.05 $&$ 3.8\pm0.3   $&$ 0.05\pm0.09$& [1]\\
\object{HD~52919 }&$ 4740\pm49  $&$ 4.25\pm0.1  $&$ 1.03\pm0.09 $&$ -0.05\pm0.06$ &$ 4.8\pm1.0 $&$-0.04\pm0.11$&[3]\\
\object{HD~53143 }&$ 5462\pm54  $&$ 4.47\pm0.07 $&$ 1.08\pm0.07 $&$  0.22\pm0.06$ &$ 1.9\pm0.5 $&$-0.25\pm0.14$&[3]\\
\object{HD~67199 }&$ 5136\pm56  $&$ 4.54\pm0.08 $&$ 0.84\pm0.08 $&$  0.06\pm0.06$ &$ 6.3\pm2.0 $&$ 0.28\pm0.18$&[3]\\
\object{HD~100623}&$ 5246\pm37  $&$ 4.54\pm0.05 $&$ 1   \pm0.06 $&$ -0.38\pm0.05$ &$ 2.3\pm0.5 $&$-0.32\pm0.10$&[3]\\
\object{HD~102365}&$ 5667\pm27  $&$ 4.59\pm0.02 $&$ 1.05\pm0.06 $&$ -0.27\pm0.04$ &$ 3.8\pm0.5 $&$-0.04\pm0.07$&[3]\\
\object{HD~104304}&$ 5562\pm50  $&$ 4.37\pm0.06 $&$ 1.1 \pm0.06 $&$  0.27\pm0.06$ &$ 6.0\pm0.5 $&$ 0.22\pm0.05$&[3]\\
\object{HD~109200}&$ 5103\pm46  $&$ 4.47\pm0.07 $&$ 0.75\pm0.07 $&$ -0.24\pm0.05$ &$ 5.2\pm0.4 $&$ 0.06\pm0.05$&[3]\\
\object{HD~115617}&$ 5577\pm33  $&$ 4.34\pm0.03 $&$ 1.07\pm0.04 $&$  0.01\pm0.05$ &$ 4.6\pm1.0 $&$ 0.00\pm0.11$&[3]\\
\object{HD~118972}&$ 5241\pm66  $&$ 4.43\pm0.1  $&$ 1.24\pm0.08 $&$ -0.01\pm0.08$ &$ 3.6\pm0.9 $&$-0.06\pm0.19$&[3]\\
\object{HD~125072}&$ 5001\pm115 $&$ 4.39\pm0.21 $&$ 1.21\pm0.15 $&$  0.24\pm0.11$ &$ 8.3\pm1.0 $&$ 0.39\pm0.12$&[3]\\
\object{HD~140901}&$ 5645\pm37  $&$ 4.4 \pm0.04 $&$ 1.14\pm0.05 $&$  0.13\pm0.05$ &$ 6.2\pm1.5 $&$ 0.21\pm0.12$&[3]\\
\object{HD~144628}&$ 5071\pm43  $&$ 4.41\pm0.06 $&$ 0.82\pm0.07 $&$ -0.36\pm0.06$ &$ 6.5\pm0.8 $&$ 0.09\pm0.07$&[3]\\
\object{HD~146233}&$ 5786\pm35  $&$ 4.31\pm0.03 $&$ 1.18\pm0.05 $&$  0.08\pm0.05$ &$ 7.7\pm1.0 $&$ 0.26\pm0.07$&[3]\\
\object{HD~152391}&$ 5521\pm43  $&$ 4.54\pm0.05 $&$ 1.29\pm0.06 $&$  0.03\pm0.05$ &$ 4.7\pm0.7 $&$ 0.12\pm0.08$&[3]\\
\object{HD~154088}&$ 5414\pm60  $&$ 4.28\pm0.08 $&$ 1.14\pm0.07 $&$  0.33\pm0.07$ &$ 6.6\pm0.7 $&$ 0.25\pm0.07$&[3]\\
\object{HD~156274}&$ 5300\pm32  $&$ 4.41\pm0.04 $&$ 1   \pm0.05 $&$ -0.33\pm0.05$ &$ 5.0\pm0.9 $&$-0.02\pm0.09$&[3]\\
\object{HD~165499}&$ 5950\pm45  $&$ 4.31\pm0.02 $&$ 1.14\pm0.08 $&$  0.01\pm0.06$ &$ 4.5\pm1.0 $&$ 0.01\pm0.10$&[3]\\
\object{HD~170657}&$ 5115\pm52  $&$ 4.48\pm0.08 $&$ 1.13\pm0.07 $&$ -0.22\pm0.06$ &$ 4.0\pm0.5 $&$-0.05\pm0.07$&[3]\\
\object{HD~172051}&$ 5634\pm30  $&$ 4.43\pm0.03 $&$ 1.06\pm0.05 $&$ -0.20\pm0.04$ &$ 4.7\pm0.5 $&$-0.01\pm0.05$&[3]\\
\object{HD~177565}&$ 5664\pm28  $&$ 4.43\pm0.02 $&$ 1.02\pm0.04 $&$  0.14\pm0.04$ &$ 6.2\pm0.5 $&$ 0.23\pm0.04$&[3]\\
\object{HD~192310}&$ 5069\pm49  $&$ 4.38\pm0.19 $&$ 0.79\pm0.07 $&$ -0.01\pm0.05$ &$ 4.5\pm0.5 $&$ 0.03\pm0.11$&[4]\\
\object{HD~222335}&$5260\pm41 $ & $ 4.45\pm0.11$ &$ 0.92\pm0.06 $&$ -0.16\pm0.05 $&$ 8.0\pm1.0 $&$ 0.27\pm0.07$&\ [3]\\
\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}