\begin{table}%t1
\caption{Observational details of the telescope/instrument combinations used for
this paper. The second column presents the complete wavelength coverage of the data,
whilst the numbers in parentheses are the number of wavelength settings required to obtain this
coverage. The third and fourth columns display the mean signal-to-noise ($S/N$) ratio 
and resolution of the data.}\label{obs}   
\small%\begin{center}
{
\begin{tabular}{lccc} 
\hline \hline
%&&& \\[-8pt]
Telescope/Instrument	& $\lambda$-range (\AA)	 & $S/N$ & $R$ \\	  
\hline   
\\
VLT/FLAMES	& 3850--4755, 6380--6620             (6) & 100--150 & 20~000--30~000\\  	
VLT/UVES$^{1}$  & 3750--5000, 5900--7700, 7750--9600  (3) & 40      & 20~000\\
ESO2.2 m/FEROS   & 3600--9300                        (1) & $>$100  & 48~000\\
\hline 
\end{tabular}}
{
$^{1}$ UVES data only used for one object NGC330-124.}
%\end{center}
\par
\end{table}