\begin{table}%t14
%\centering
\small
\caption{NGC~3960: comparison with the results by Bragaglia
et~al.~(\cite{bragaglia06}); numbers
in parenthesis are their IDs.}\label{confr}
\begin{tabular}{lllllll}
\hline
\hline
star & & $T_{\rm{eff}}$ & log $g$ & $\xi$ & [Fe/H] & $\Delta{\log n(\rm{Fe})}$ \\
 & & K & & km s$^{-1}$ \\
\hline
%&&&&& \\[-3.2mm]
c5     &MOOG & 4870 &2.16 & 1.22 &+0.00   &$-$0.09 \\
(41)   &ROSA & 4850 &2.20 & 1.21 &$-$0.14 &        \\
%&&&&& \\
c6     &MOOG & 4950 &2.40 & 1.19 &+0.02   &$-$0.12 \\
(28)   &ROSA & 4900 &2.06 & 1.23 &$-$0.15 &        \\
%&&&&& \\
c8     &MOOG & 5040 &2.57 & 1.17 &+0.00   &$-$0.01 \\
(50)   &ROSA & 5000 &2.70 & 1.15 &$-$0.06 &        \\
\hline
\end{tabular}
\end{table}