\begin{table} %ta.2 
%\centering
\par
\caption{Radial velocities, effective temperatures, and lithium abundances of the 59 stars retained as possible single members. The values in Table are derived by adding the difference of $T_{\rm eff}$ between the stars and the Sun to the solar temperature (5777 K). The solar temperature derived  from the GIRAFFE spectrum and our calibrations is  5792 and 5717~K for the LDR and H$\alpha$ methods, respectively. The 10 best solar twin candidates are indicated in bold face. The $S/N$ /pixel of the co-added spectra varies between 80 and 110, depending on the magnitude of the stars.}
\label{tab:targets_selected}
%\scriptsize
\begin{tabular}{lcclrrcr}
\hline\hline\noalign{\smallskip}
Object & $V_{\rm rad}\pm\Delta V_{\rm rad}$ & $T_{\rm eff}^{\rm LDR}\pm\Delta T_{\rm eff}^{\rm LDR}$ & $T_{\rm eff}^{\rm H\alpha}$ & $EW_{\rm Li+Fe}$ &
$\log EW_{\rm Li}$ & $\log N{\rm (Li)}^{\rm LTE}$ & $\log N{\rm (Li)}^{\rm NLTE}$ \\
       & (km~s$^{-1}$) & ($K$)& ($K$) & (m\AA) & (m\AA) &    &\\ 
\hline
Sun    &                 & $5777\pm27$ & 5777 &  12.1  &     0.3&  0.8  &  0.8	   \\
219    &  $33.85\pm0.28$ & $6243\pm54$ & 6110 &  22.7  &     1.2&  2.1  &  2.1     \\
266    &  $32.95\pm0.46$ & $6147\pm63$ & 6060 &  53.2  &     1.7&  2.6  &  2.5     \\
{\bf 285 }   &  $33.72\pm0.67$ & $5836\pm67$ & 5777 &   1.5  & $<$0.0&  0.6  &  $<$0.6 \\
288    &  $34.26\pm0.40$ & $6004\pm67$ & 6010 &  42.4  &     1.5&  2.3  &  2.3     \\
291    &  $32.13\pm0.29$ & $6177\pm57$ & 6160 &  59.6  &     1.7&  2.6  &  2.6     \\
349    &  $34.28\pm0.42$ & $5952\pm78$ & 5917 &  10.4  & $<$0.0&  0.7  &  $<$0.7 \\
350    &  $32.56\pm0.31$ & $6024\pm52$ & 6010 &  68.2  &     1.8&  2.6  &  2.6     \\
401    &  $32.64\pm0.37$ & $6165\pm64$ & 6110 &  44.9  &     1.6&  2.5  &  2.4     \\
473    &  $34.74\pm0.38$ & $5919\pm76$ & 5807 &   2.7  & $<$0.0&  0.7  &  $<$0.7 \\
587    &  $33.06\pm0.39$ & $6077\pm65$ & 6060 &  37.2  &     1.4&  2.3  &  2.3     \\
613    &  $33.05\pm0.29$ & $6202\pm45$ & 6110 &  61.3  &     1.7&  2.7  &  2.6     \\
{\bf 637  }  &  $34.00\pm0.50$ & $5806\pm65$ & 5777 &  17.8  &     0.9&  1.4  &  1.4    \\
673    &  $32.44\pm0.57$ & $5639\pm63$ & 5747 &  19.1  &     0.9&  1.4  &  1.4     \\
689    &  $32.88\pm0.24$ & $6093\pm41$ & 6110 &  42.3  &     1.5&  2.4  &  2.3     \\
%713    &  $35.09\pm0.29$ & $5833\pm52$ & 5867 &  29.6  &     1.3&  1.9  &  1.9     \\
750    &  $33.13\pm0.28$ & $5918\pm48$ & 5927 &  16.4  &     0.9&  1.5  &  1.5     \\
769    &  $34.47\pm0.29$ & $5984\pm46$ & 6010 &  29.4  &     1.3&  2.1  &  2.0     \\
778    &  $33.45\pm0.24$ & $6114\pm39$ & 6060 &  15.6  &     0.8&  1.7  &  1.7     \\
809    &  $31.87\pm0.48$ & $5667\pm78$ & 5537 &   6.9  & $<$0.0&  0.4  &  $<$0.5 \\
851    &  $33.47\pm0.31$ & $5948\pm61$ & 6060 &  12.9  &     0.6&  1.3  &  1.3     \\
911    &  $32.08\pm0.35$ & $5885\pm67$ & 5837 &  13.4  &     0.6&  1.2  &  1.2     \\
988    &  $32.07\pm0.28$ & $5935\pm53$ & 6060 &  28.2  &     1.3&  2.0  &  2.0     \\
1032   &  $34.02\pm0.47$ & $5955\pm60$ & 6010 &  17.8  &     0.9&  1.6  &  1.6     \\
1036   &  $33.39\pm0.48$ & $5612\pm66$ & 5537 &  20.9  &     1.0&  1.4  &  1.4     \\
1051   &  $32.21\pm0.29$ & $6081\pm55$ & 6060 &  34.7  &     1.4&  2.2  &  2.2     \\
1062   &  $32.64\pm0.45$ & $5926\pm55$ & 5867 &  21.0  &     1.1&  1.7  &  1.7     \\
1067   &  $33.37\pm0.35$ & $5929\pm69$ & 5917 &  11.4  &     0.4&  1.0  &  1.0     \\
1075   &  $33.13\pm0.24$ & $5871\pm48$ & 5917 &  10.7  &     0.0&  0.6	&  0.7	   \\
1088   &  $32.87\pm0.29$ & $5890\pm59$ & 5867 &   9.3  & $<$0.0&  0.6  &  $<$0.7 \\
1090   &  $33.34\pm0.32$ & $6086\pm54$ & 6010 &  41.2  &     1.5&  2.3  &  2.3	   \\
{\bf 1101}   &  $32.72\pm0.34$ & $5756\pm60$ & 5717 &   6.9  & $<$0.0&  0.5  &  $<$0.6 \\
1129   &  $33.92\pm0.30$ & $5959\pm51$ & 6010 &  32.4  &     1.4&  2.1  &  2.1     \\
1137   &  $33.59\pm0.48$ & $5741\pm69$ & 5627 &   5.3  & $<$0.0&  0.5  &  $<$0.6 \\
{\bf 1194}   &  $33.30\pm0.40$ & $5766\pm64$ & 5837 &   5.3  & $<$0.0&  0.5  &  $<$0.6 \\
1197   &  $34.26\pm0.28$ & $6207\pm44$ & 6110 &  28.1  &     1.3&  2.2  &  2.2     \\
1247   &  $32.44\pm0.51$ & $5994\pm60$ & 6010 &  30.2  &     1.3&  2.1  &  2.1     \\
{\bf 1303 }  &  $32.65\pm0.41$ & $5716\pm64$ & 5717 &  10.1  & $<$0.0&  0.5  &  $<$0.6 \\
{\bf 1304  } &  $33.60\pm0.39$ & $5704\pm64$ & 5717 &   7.9  & $<$0.0&  0.5  &  $<$0.5 \\
{\bf 1315   }&  $32.55\pm0.34$ & $5874\pm58$ & 5867 &  15.6  &     0.8&  1.4  &  1.4    \\
1334   &  $32.37\pm0.45$ & $5957\pm57$ & 5957 &  29.2  &     1.3&  2.0  &  2.0     \\
1387   &  $33.35\pm0.24$ & $6090\pm58$ & 6060 &  37.5  &     1.5&  2.3  &  2.3     \\
{\bf 1392}   &  $33.68\pm0.57$ & $5716\pm63$ & 5687 &   6.3  & $<$0.0&  0.5  &  $<$0.6 \\
%1397   &  $35.07\pm0.50$ & $6127\pm33$ & 6110 &  35.7  &     1.4&  2.3  &  2.3     \\
1458   &  $32.55\pm0.56$ & $5640\pm65$ & 5567 &   6.1  & $<$0.0&  0.4  &  $<$0.5 \\
1496   &  $34.22\pm0.48$ & $6173\pm54$ & 6160 &  63.1  &     1.7&  2.7  &  2.6     \\
1504   &  $33.39\pm0.48$ & $5934\pm56$ & 6060 &  40.7  &     1.5&  2.2  &  2.2     \\
1514   &  $33.33\pm0.49$ & $5613\pm67$ & 5597 &  25.6  &     1.2&  1.6  &  1.6     \\
1587   &  $32.38\pm0.62$ & $5975\pm55$ & 6010 &  28.6  &     1.3&  2.0  &  2.0     \\
1622   &  $33.26\pm0.61$ & $6043\pm57$ & 6010 &  34.6  &     1.4&  2.2  &  2.2     \\
1716   &  $33.84\pm0.59$ & $6030\pm40$ & 6060 &  40.8  &     1.5&  2.3  &  2.3     \\
1722   &  $33.87\pm0.52$ & $6007\pm62$ & 6010 &  38.1  &     1.5&  2.3  &  2.2     \\
1735   &  $33.18\pm0.59$ & $5959\pm59$ & 5960 &  10.9  &     0.2&  0.9  &  0.9     \\
1758   &  $33.78\pm0.67$ & $6221\pm52$ & 6160 &  36.3  &     1.4&  2.4  &  2.4     \\
1768   &  $33.98\pm0.57$ & $5844\pm57$ & 5927 &  40.1  &     1.5&  2.1  &  2.1     \\
{\bf 1787 }  &  $33.44\pm0.57$ & $5768\pm70$ & 5807 &  12.9  &     0.5&  1.1  &  1.0   \\
1788   &  $33.38\pm0.80$ & $5886\pm60$ & 5867 &  23.4  &     1.1&  1.8  &  1.8     \\
1852   &  $32.30\pm0.40$ & $6009\pm63$ & 6010 &  32.2  &     1.4&  2.1  &  2.1     \\
1903   &  $32.76\pm0.42$ & $5609\pm72$ & 5687 &   6.8  & $<$0.0&  0.4  &  $<$0.5 \\
1948   &  $32.86\pm0.29$ & $6164\pm63$ & 6010 &  43.0  &     1.5&  2.4  &  2.4     \\
1955   &  $32.63\pm0.60$ & $5961\pm76$ & 5837 &  35.8  &     1.4&  2.2  &  2.2     \\
{\bf 2018}   &  $31.78\pm0.43$ & $5693\pm74$ & 5777 &   8.7  & $<$0.0&  0.4  &  $<$0.5 \\
\hline
\end{tabular}
\end{table}