\begin{table}%t2
%\centering
\par
\caption{\label{spectradata}Stellar data derived with spectroscopic analysis.}
\begin{tabular}{ccccccccc}
\hline\hline\noalign{\smallskip}
ID & $\frac{S}{N}$ & $T_{\rm eff}$ & $\log{g}$ & [$\frac{{\rm Fe}}{{\rm H}}$] & $v_{\rm t}$ & RV & $E(B-V$) & $d$ \\
 & & K & dex & dex & km s$^{-1}$ & km s$^{-1}$ & mag & pc \\
\hline
4 & 25 & 4110 $\pm$ 65 & 1.05 $\pm$ 0.20 & $-$0.62 $\pm$ 0.08 & 1.28 $\pm$ 0.20 & --55.1 $\pm$ 0.3 & 0.23 $\pm$ 0.05 & 6800 $\pm$ 1100 \\
5 & 15 & 5440 $\pm$ 65 & 3.55 $\pm$ 0.20 & $-$0.09 $\pm$ 0.08 & 0.65 $\pm$ 0.20 &  21.6 $\pm$ 0.5 & 0.30 $\pm$ 0.05 & 1270 $\pm$ 280 \\
7 & 10 & 6100 $\pm$ 75 & 4.45 $\pm$ 0.20 & $-$0.06 $\pm$ 0.09 & 1.32 $\pm$ 0.15 &  35.3 $\pm$ 0.4 & 0.34 $\pm$ 0.04 &  560 $\pm$ 50 \\
8 & 10 & 5320 $\pm$ 65 & 3.85 $\pm$ 0.10 & $-$0.41 $\pm$ 0.10 & 1.24 $\pm$ 0.15 & --10.6 $\pm$ 0.5 & 0.26 $\pm$ 0.05 &  740 $\pm$ 90 \\
\hline
\end{tabular}
\end{table}