\begin{table}%t3
\caption{Stellar properties for the new Taurus members and the uncertain sources observed with DOLORES.}\label{tab:stars_lrs_memb_unc}
\par
\small%\centerline
 {
\begin{tabular}{lccccccc}
\hline\hline
%&&&&&&& \\[-8pt]
Star        & Sp. type$^a$ & H$\alpha$ {\it EW}$^a$ & $A_{\rm V}~^b$ & $N_{\rm H}~^c$ & $M$ & Age (range) & Evol. stage \\ 
            &  &      (\AA\ )      &      (mag)      & ($10^{21}$~cm$^{-2}$) & ($M_{\odot}$) & (Myr) &      \\ 
            \hline
\multicolumn{8}{c}{new TMC members} \\
\object{XEST-08-033} & M2 IV    & --11   & $1.8\pm 0.1$ & $4.0\pm 1.0$   & $0.35^{+0.1}_{-0.15}$ & $5\ (1{-}10)$  & WTTS \\ 
\object{XEST-08-047} & M2 IV    &  --6   & $3.2\pm 0.3$ &                & $0.50^{+0.1}_{-0.05}$ & $7\ (5{-}10)$   & WTTS \\ 
\object{XEST-08-049} & M2 IV    &  --9   & $1.8\pm 0.2$ & $3.0\pm 0.2$   & $0.50^{+0.05}_{-0.15}$ & $5\ (3{-}10)$     & WTTS \\ 
\object{XEST-11-078} & K2-4 V    & --16.5 & -- &                & -- & -- & CTTS \\ 
\object{XEST-11-087}$^d$ & M3 IV    &  --6   & $2.0\pm 0.2$ &                & $0.25\pm 0.1$ & $3\ (1{-}5)$ & WTTS \\ 
\object{XEST-16-045} & M3/4 IV  & --8.5  & $0 ({<}0.1)$  &                & $0.30\pm 0.1$ & $3\ (1{-}5)$ & WTTS \\ 
\object{XEST-17-059} & M5 IV    & --16   & $0.6\pm 0.1$ & $1.8\pm 0.3$  & $0.20\pm0.05$ & $1 ({<}3)$ & WTTS \\ 
\hline
\multicolumn{8}{c}{uncertain stars} \\
\object{XEST-08-014}$^e$ & M2/3  & --8.5  & $\sim$$0$      & $\la$$0.2$ & 0.4  & $\sim$$10$  & WTTS or MS at $\sim$$65$ pc \\ 
\object{XEST-15-034}$^e$ & M4 V      & --5    & $\sim$$0{-}0.15$ & $\la$$0.2$ & 0.35 & $\ga$$10$ & WTTS or MS at $\sim$$120$ pc \\ 
\object{XEST-20-071} & M?        & --6    & -- & $4.1\pm 0.4$   & -- & -- & ? \\ 
\hline
\end{tabular}}
\medskip
$^a$ From low-resolution spectra (Sect.~\ref{dolores});
$^b$ from IR color$-$color diagram (Sect.~\ref{IRdiagr_lrs});
$^c$ from X-ray spectral fitting \citep{ScelsiXEST2006};
$^d$ possible IR excess may affect the $A_{\rm V}$, mass and age values;
$^e$ values of $A_{\rm V}$, $M$ and age refer to the PMS case and are not confirmed. 
\end{table}