\begin{table}%T13
\caption{Comparison of measured {\it EW} of \ion{C}{i} line at 5380~\AA\ from 
our data and from other authors. }\label{tab12}
%\centerline
{
\begin{tabular}{lccccccr}
\hline
\hline
Star & $T_{\rm eff}$ & $\log {g}$       & $\xi_t$   & [Fe/H]  & {\it EW} & ${\it EW}_{\rm liter}$ & Ref. \\
     & (K)              &  (cm~s$^{-2}$) & (km~s$^{-1}$) &  &  &  &  \\
\hline 
\object{HD~1237}   & $5536\pm50$ & $4.56\pm0.12$ & $1.33\pm0.06$ & $ 0.12\pm0.06$ & $16.7$ & $17.0$ & 1 \\
\object{HD~9826}   & $6212\pm64$ & $4.26\pm0.13$ & $1.69\pm0.16$ & $ 0.13\pm0.08$ & $45.2$ & $41.5$ & 3 \\
\object{HD~10697}  & $5641\pm28$ & $4.05\pm0.05$ & $1.13\pm0.03$ & $ 0.14\pm0.04$ & $27.4$ & $24.9$ & 2 \\
\object{HD~12661}  & $5702\pm36$ & $4.33\pm0.08$ & $1.05\pm0.04$ & $ 0.36\pm0.05$ & $32.3$ & $31.9$ & 2K \\
\object{HD~13445}  & $5163\pm00$ & $4.52\pm0.00$ & $0.72\pm0.00$ & $-0.24\pm0.00$ & $12.9$ & $ 7.8$ & 1 \\
\object{HD~22049}  & $5073\pm42$ & $4.43\pm0.08$ & $1.05\pm0.06$ & $-0.13\pm0.05$ & $ 9.5$ & $ 9.8$ & 3 \\
\object{HD~37124}  & $5546\pm30$ & $4.50\pm0.03$ & $0.80\pm0.07$ & $-0.38\pm0.04$ & $13.0$ & $11.9$ & 2K \\
\object{HD~38529}  & $5674\pm40$ & $3.94\pm0.12$ & $1.38\pm0.05$ & $ 0.40\pm0.06$ & $45.0$ & $35.2$ & 2K \\ 
\object{HD~38529}  & $5674\pm40$ & $3.94\pm0.12$ & $1.38\pm0.05$ & $ 0.40\pm0.06$ & $45.0$ & $35.5$ & 3 \\ 
\object{HD~46375}  & $5268\pm55$ & $4.41\pm0.16$ & $0.97\pm0.06$ & $ 0.20\pm0.06$ & $20.8$ & $19.7$ & 2K \\ 
\object{HD~52265}  & $6105\pm00$ & $4.28\pm0.00$ & $1.36\pm0.00$ & $ 0.23\pm0.00$ & $43.6$ & $39.4$ & 1 \\
\object{HD~52265}  & $6105\pm00$ & $4.28\pm0.00$ & $1.36\pm0.00$ & $ 0.23\pm0.06$ & $43.6$ & $41.6$ & 2K \\
\object{HD~52265}  & $6105\pm00$ & $4.28\pm0.00$ & $1.36\pm0.00$ & $ 0.23\pm0.06$ & $43.6$ & $37.1$ & 3 \\
\object{HD~75289}  & $6143\pm53$ & $4.42\pm0.13$ & $1.53\pm0.09$ & $ 0.28\pm0.07$ & $37.6$ & $39.0$ & 1 \\
\object{HD~75732}  & $5279\pm62$ & $4.37\pm0.18$ & $0.98\pm0.07$ & $ 0.33\pm0.07$ & $21.6$ & $19.5$ & 3 \\ 
\object{HD~82943}  & $6015\pm00$ & $4.46\pm0.00$ & $1.13\pm0.00$ & $ 0.30\pm0.00$ & $37.6$ & $35.4$ & 4 \\
\object{HD~82943}  & $6015\pm00$ & $4.46\pm0.00$ & $1.13\pm0.00$ & $ 0.30\pm0.00$ & $37.6$ & $36.3$ & 1 \\
\object{HD~83443}  & $5454\pm61$ & $4.33\pm0.17$ & $1.08\pm0.08$ & $ 0.35\pm0.08$ & $27.7$ & $26.1$ & 1 \\ 
\object{HD~89744}  & $6234\pm45$ & $3.98\pm0.05$ & $1.62\pm0.08$ & $ 0.22\pm0.05$ & $50.2$ & $49.3$ & 2 \\ 
\object{HD~89744}  & $6234\pm45$ & $3.98\pm0.05$ & $1.62\pm0.08$ & $ 0.22\pm0.05$ & $50.2$ & $43.0$ & 3 \\
\object{HD~92788}  & $5821\pm41$ & $4.45\pm0.06$ & $1.16\pm0.05$ & $ 0.32\pm0.05$ & $37.0$ & $31.1$ & 2K \\
\object{HD~92788}  & $5821\pm41$ & $4.45\pm0.06$ & $1.16\pm0.05$ & $ 0.32\pm0.05$ & $37.0$ & $28.8$ & 4 \\
\object{HD~95128}  & $5954\pm25$ & $4.44\pm0.10$ & $1.30\pm0.04$ & $ 0.06\pm0.03$ & $25.9$ & $25.8$ & 3 \\
\object{HD~106252} & $5899\pm35$ & $4.34\pm0.07$ & $1.08\pm0.06$ & $-0.01\pm0.05$ & $23.1$ & $21.8$ & 4 \\
\object{HD~114762} & $5884\pm34$ & $4.22\pm0.22$ & $1.31\pm0.17$ & $-0.70\pm0.04$ & $12.2$ & $10.0$ & 4 \\
\object{HD~117176} & $5560\pm34$ & $4.07\pm0.05$ & $1.18\pm0.05$ & $-0.06\pm0.05$ & $18.0$ & $14.9$ & 3 \\
\object{HD~120136} & $6339\pm73$ & $4.19\pm0.10$ & $1.70\pm0.16$ & $ 0.23\pm0.07$ & $59.9$ & $56.8$ & 3 \\ 
\object{HD~130322} & $5392\pm36$ & $4.48\pm0.06$ & $0.85\pm0.05$ & $ 0.03\pm0.04$ & $14.5$ & $14.6$ & 2 \\
\object{HD~130322} & $5392\pm36$ & $4.48\pm0.06$ & $0.85\pm0.05$ & $ 0.03\pm0.04$ & $14.5$ & $13.7$ & 4 \\
\object{HD~134987} & $5776\pm29$ & $4.36\pm0.07$ & $1.09\pm0.04$ & $ 0.30\pm0.04$ & $36.3$ & $34.8$ & 2 \\
\object{HD~134987} & $5776\pm29$ & $4.36\pm0.07$ & $1.09\pm0.04$ & $ 0.30\pm0.04$ & $36.3$ & $34.1$ & 4 \\
\object{HD~141937} & $5909\pm39$ & $4.51\pm0.08$ & $1.13\pm0.06$ & $ 0.10\pm0.05$ & $28.2$ & $26.5$ & 4 \\
\object{HD~143761} & $5853\pm25$ & $4.41\pm0.15$ & $1.35\pm0.07$ & $-0.21\pm0.04$ & $21.1$ & $15.9$ & 3 \\
\object{HD~145675} & $5311\pm87$ & $4.42\pm0.18$ & $0.92\pm0.10$ & $ 0.43\pm0.08$ & $24.5$ & $23.9$ & 3 \\ 
\object{HD~168443} & $5617\pm35$ & $4.22\pm0.05$ & $1.21\pm0.05$ & $ 0.06\pm0.05$ & $26.7$ & $27.3$ & 2 \\
\object{HD~168746} & $5601\pm33$ & $4.41\pm0.12$ & $0.99\pm0.05$ & $-0.08\pm0.05$ & $22.5$ & $18.0$ & 4 \\
\object{HD~169830} & $6299\pm41$ & $4.10\pm0.02$ & $1.42\pm0.09$ & $ 0.21\pm0.05$ & $48.2$ & $45.1$ & 1 \\
\object{HD~186427} & $5772\pm25$ & $4.40\pm0.07$ & $1.07\pm0.04$ & $ 0.08\pm0.04$ & $23.8$ & $23.9$ & 3 \\
\object{HD~187123} & $5845\pm22$ & $4.42\pm0.07$ & $1.10\pm0.03$ & $ 0.13\pm0.03$ & $26.2$ & $24.9$ & 4 \\
\object{HD~190228} & $5325\pm00$ & $3.90\pm0.00$ & $1.11\pm0.00$ & $-0.26\pm0.00$ & $12.6$ & $11.9$ & 4 \\
\object{HD~202206} & $5752\pm53$ & $4.50\pm0.09$ & $1.01\pm0.06$ & $ 0.35\pm0.06$ & $27.1$ & $22.5$ & 1 \\
\object{HD~217014} & $5804\pm36$ & $4.42\pm0.07$ & $1.20\pm0.05$ & $ 0.20\pm0.05$ & $34.3$ & $30.2$ & 2 \\
\object{HD~217014} & $5804\pm36$ & $4.42\pm0.07$ & $1.20\pm0.05$ & $ 0.20\pm0.05$ & $34.3$ & $29.5$ & 3 \\
\object{HD~217107} & $5645\pm00$ & $4.31\pm0.00$ & $1.06\pm0.00$ & $ 0.37\pm0.00$ & $29.1$ & $27.6$ & 2 \\ 
\object{HD~217107} & $5645\pm00$ & $4.31\pm0.00$ & $1.06\pm0.00$ & $ 0.37\pm0.00$ & $29.1$ & $29.4$ & 3 \\
\object{HD~222582} & $5843\pm38$ & $4.45\pm0.07$ & $1.03\pm0.06$ & $ 0.05\pm0.05$ & $22.2$ & $20.1$ & 2 \\\hline
\end{tabular}}
\par
\medskip
\par
$^1$ From Santos et~al. (\cite{San00}).\\
$^2$ From Gonzalez et~al. (\cite{Gonz01}); 2K refers to data from Keck
spectra.\\
$^3$ From Takeda et~al.\ (\cite{Tak01}).\\
$^4$ From Sadakane et~al.\ (\cite{Sad02}).
\end{table}