\begin{table}%T1
\caption{\ion{Fe}{i} lines used for setting the wavelength scale in the stellar spectrum and determining the rotational velocity.}
\label{fetab}
%\centerline
 {\small
\begin{tabular}{l c c}
\hline\hline\\[-3.2mm]
$\lambda_{\rm air}$ (\AA) & Ref.$^a$ & log \emph{gf}$^b$ \\
\hline
4592.6512 & LT & --2.449 \\  
4602.9409 & LT & --2.250 \\  
4691.412 & TW & --1.450 \\    
4710.2834 & LT & --1.612 \\    
5049.8196 & LT & --1.420 \\  
5051.635 & TW & --2.795 \\    
5068.7657 & LT & --1.055 \\    
5098.6959 & LT & --2.026 \\  
5107.448 & TW & --3.087 \\  
5107.641 & TW$^c$ & --2.418 \\  
5110.413 & TW & --3.760 \\
\hline
\end{tabular}}
\medskip
\par
$^a$ TW: This work; LT: \cite{Learner88}; $^b$ \cite{Kurucz95}; $^c$ blended with \ion{Nd}{ii} line in stellar spectrum. 
\end{table}