\begin{table}%t3
%\centering
\par
\caption{Observed parameters of the new T Tauri stars.\label{params}}
\begin{tabular}{lcrcccccccrrc}
\hline \hline
No & GSC & \multicolumn{1}{c}{$W$(H$\alpha$)} & $W$(Li)$^1$ & $W$(\ion{Na}{i}) 
& $W$(\ion{Ca}{i}) & $V$ & $I_{\rm C}$ & $V-I_{\rm C}$ & Sp & 
\multicolumn{1}{c}{$m_{\rm bol}$} & \multicolumn{1}{c}{$\log L_{{\rm bol}}$} & log\\
 & name & \multicolumn{1}{c}{(5653) [\AA]} & (6708) [\AA] & (5890) [\AA] & 
(6161) [\AA] & [mag] & [mag] & [mag] & types & \multicolumn{1}{c}{[mag]} & 
\multicolumn{1}{c}{[$L_{\odot}$]} & $L_{\rm X}/L_{\rm bol}$\\
\hline
4c1 & \object{0450001478} & 0.7 & 0.4 & 2.5 & 1.1 & 10.43 & 9.50 & 0.92 & K1 & 10.06 & 0.48 & $-3.41$\\
4c2 & & -1.9 & 0.4 & 6.0 & 2.2 & 13.86 & 12.09 & 1.77 & K7 & 12.94 & -0.68 & $-2.26$\\
5c1 & \object{0450001549} & -1.6 & 0.5 & 7.4 & 3.0 & 12.18 & 10.66 & 1.52 & K6 & 11.36 & -0.04 & $-2.80$\\
5c2 & & & & & & 14.12 & 12.03 & 2.10 & M2$^2$ & 12.48 & -0.49 & $-2.35$\\
19 & \object{0458901101} & -3.4 & 0.4 & 1.5 & 0.8 & 10.39 & 9.57 & 0.82 & G8 & 10.14 & 0.44 & $-3.85$\\
20 & \object{0445900083} & 0.9 & 0.4 & 1.5 & 0.8 & 10.62 & 9.78 & 0.84 & K0 & 10.31 & 0.37 & $-3.04$\\
28 & \object{0458601090} & 1.2 & 0.3 & 1.5 & 0.8 & 11.66 & 10.85 & 0.81 & G8 & 11.41 & -0.06 & $-3.09$\\
34 & \object{0460801986} & -3.0 & 0.5 & 5.6 & 2.1 & 13.09 & 11.53 & 1.55 & K7 & 12.17 & -0.37 & $-2.92$\\
36c1 & \object{0427200174} & 0.9 & 0.5 & 2.0 & 1.1 & 12.92 & 11.79 & 1.13 & K4 & 12.37 & -0.45 & $-2.85$\\
36c2 & & & & & & 14.69 & 11.85 & 2.84 & M4$^2$ & 12.13 & -0.36 & $-2.95$\\
37c1 & \object{0448000917} & 0.4 & 0.6 & 2.1 & 0.8 & 11.63 & 9.98 & 1.65 & K3 & 9.70$^4$ & 0.62 & $-3.88$\\
37c2 & & & & & & 14.86 & 13.75 & 1.12 & F4$^3$ & 13.30$^4$ & -0.82 & $-2.43$\\
38 & \object{0460400743} & 0.0 & 0.5 & 2.2 & 1.2 & 11.88 & 10.86 & 1.03 & K2 & 11.46 & -0.09 & $-3.22$\\
40 & \object{0460502733} & 1.2 & 0.4 & 1.6 & 1.0 & 10.98 & 10.10 & 0.88 & K0 & 10.67 & 0.23 & $-3.17$\\
41 & \object{0460500268} & -1.8 & 0.4 & 4.4 & 2.1 & 13.19 & 11.60 & 1.59 & K6 & 12.37 & -0.45 & $-2.75$\\
43c1 & \object{0448900036} & -4.3 & 0.5 & 5.5 & 2.8 & 13.21 & 11.35 & 1.86 & K7 & 12.29 & -0.42 & $-2.75$\\
43c2 & & & & & & 15.55 & 13.05 & 2.50 & M3$^2$ & 13.52 & -0.91 & $-2.26$\\
44 & \object{0460500170} & -0.6 & 0.5 & 3.9 & 1.6 & 11.77 & 10.54 & 1.24 & K4 & 11.22 & 0.01 & $-2.60$\\
45 & \object{0447900348} & -0.1 & 0.4 & 1.9 & 1.3 & 12.64 & 11.64 & 1.00 & K2 & 12.22 & -0.39 & $-2.79$\\
46 & \object{0461001318} & 0.9 & 0.4 & 1.9 & 1.0 & 11.34 & 10.41 & 0.93 & K1 & 10.97 & 0.11 & $-3.22$\\
\hline
\noalign{\smallskip}
\multicolumn{13}{l}{$^1$ Up to 0.14 \AA\ have to be subtracted due
to blending 
with Fe lines.}\\
\multicolumn{7}{l}{$^2$ Derived only from the $V-I_{\rm C}$
colours.}\\
\multicolumn{13}{l}{$^3$ Derived from the $V-I_{\rm C}$ colour
and the 
reddening of $E(V-I_{\rm C})=0.57$ is assumed as estimated from 37c1.}\\
\multicolumn{7}{l}{$^4$ Extinction of $A_{\rm V}=1.43$ is applied.}
\end{tabular}
\end{table}