\begin{table}%tA.2
\caption{\label{CFHT-table}CFHT spectroscopic data products for M~34 candidate members F3\_0172 and F3\_0215.}
%\centering
\par
\begin{tabular}{rllccccccc}  
\hline\hline                 
Internal\tablefootmark{a} & JP96\tablefootmark{b} & $(B-V)_{o}$\tablefootmark{a} & Temp\tablefootmark{c} & HJD\tablefootmark{d}    &  RV           & \lii + \fei\tablefootmark{e} & \fei\tablefootmark{f}  & \lii 6708~\r{A}\tablefootmark{g} & $N$(Li)\tablefootmark{h} \\
Identifier     &            &                 & [K]        & [(+2~450~000)] & [km~s$^{-1}$] &  {\it EW} [m\r{A}]      & {\it EW} [m\r{A}] & {\it EW} [m\r{A}]          &         \\ \hline
F3\_0172       & JP  49     &  0.811          & 5139       & 5223.713     & --8.4          &  115              & 13          & 102                  & 2.003       \\ 
F3\_0215       & JP  41     &  0.874          & 4946       & 5223.712     & --7.4          &  153              & 14          & 139                  & 1.985       \\
\hline
\end{tabular} \\
\tablefoot {\tablefoottext{a}{Data taken from Tables~\ref{table-identifier} and~\ref{table-Prot};}
\tablefoottext{b}{{\em JP} identifier from Jones \& Prosser (\cite{Jone96});}
\tablefoottext{c}{temperature determined from $(B-V)_{o}$ relationship in Soberblom et~al. (1993c~-- Eq.~(3));}
\tablefoottext{d}{HJD~-- heliocentric julian date;}
\tablefoottext{e}{equivalent width measurement, by Gaussian fitting, of the blended \lii and \fei 6708~\r{A} lines;}
\tablefoottext{f}{\fei 6707.441~\r{A} line contribution, determined by an empirical ($B-V$)~colour fit (see Soderblom et~al. \cite{Sode93b});}
\tablefoottext{g}{\lii 6708~\r{A} minus the \fei 6707.441~\r{A} contribution;}
\tablefoottext{h}{Lithium equivalent widths are transformed into abundance [$N$(Li)]~-- on a scale where log~$N$(H)~=~12, using a curve of growth in Soderblom et~al. (\cite{Sode93b}).}}
\end{table}