\begin{table}%t3
\par
%\centering
\par
\caption {\label{table3}Fluxes and luminosities (first ten entries).}
\begin{tabular}{lrrrrrrrl}
\hline
\hline
\noalign{\smallskip}
Star                     & $f_{\rm [Ne~II]}$\tablefootmark{a}		         & $L_{\rm [Ne~II]}$	   &$f_{\rm X, 0.3{-}10, abs}$&$L_{\rm X, 0.3{-}10, abs}$&$f_{\rm X, 0.3{-}10, unabs}$&$L_{\rm X, 0.3{-}10, unabs}$& $N_{\rm H}$\tablefootmark{b}  & Refs.\tablefootmark{c}\\ 
                         &  (erg~cm$^{-2}$~s$^{-1}$)		 &      (erg~s$^{-1}$)	   &(erg~cm$^{-2}$~s$^{-1}$)& (erg~s$^{-1}$)         &(erg~cm$^{-2}$~s$^{-1}$)  & (erg~s$^{-1}$)           &   ($10^{22}$)  &  \\
\hline
RNO~15                   & $<$$2.6(0.85)\phantom{ }\times 10^{-14} $ & $<$$1.9\times 10^{29}$  &  $3.7\times 10^{-13}$  & $2.8\times 10^{30}$  &  $1.1\times 10^{-12}$ &  $8.0\times 10^{30}$  & 4.6       & 1, X	 \\  
LkH$\alpha$~270          & $ 1.3(0.35)\phantom{ }\times 10^{-14} $ & $ 9.7\times 10^{28}$  &  $3.2\times 10^{-13}$  & $2.4\times 10^{30}$  &  $1.5\times 10^{-12}$ &  $1.1\times 10^{31}$  & 0.78      & 1, X	     \\  
LkH$\alpha$~271          & $<$$3.6(1.2)\phantom{0}\times 10^{-15}  $ & $<$$2.7\times 10^{28}$  &  $3.8\times 10^{-14}$  & $2.8\times 10^{29}$  &  $1.1\times 10^{-13}$ &  $7.9\times 10^{29}$  & 3.8       & 1, X	     \\  
LkH$\alpha$~326          & $ 3.1(1.4)\phantom{0}\times 10^{-15}  $ & $ 2.3\times 10^{28}$  &  ...		    & ...                  &  ...	           &  ...                  & ...       & 1	     \\  
LkH$\alpha$~327          & $ 7.8(3.8)\phantom{0}\times 10^{-15}  $ & $ 5.8\times 10^{28}$  &  ...		    & ...                  &  ...	           &  ...                  & ...       & 1	     \\  
LkH$\alpha$~330          & $ 3.8(1.9)\phantom{0}\times 10^{-15}  $ & $ 2.8\times 10^{28}$  &  ...		    & ...                  &  ...	           &  ...                  & ...       & 1	     \\  
IRAS 03446+3254          & $ 4.3(0.99)\phantom{ }\times 10^{-15} $ & $ 3.2\times 10^{28}$  &  ...		    & ...                  &  ...	           &  ...                  &   ...     & 1, X	     \\  
BP~Tau                   & $ 2.9(0.4)\phantom{0}\times 10^{-15}  $ & $ 6.8\times 10^{27}$  &  $4.3\times 10^{-13}$  & $1.0\times 10^{30}$  &  $6.1\times 10^{-13}$ &  $1.4\times 10^{30}$  & 0.09      & 3, X	     \\  
FM~Tau                   & $<$$1.1(0.37)\phantom{ }\times 10^{-14} $ & $<$$2.6\times 10^{28}$  &  $1.5\times 10^{-13}$  & $3.5\times 10^{29}$  &  $2.2\times 10^{-13}$ &  $5.1\times 10^{29}$  & 0.15      & 3, X	     \\  
T~Tau N                  & $ 2.0(0.4)\phantom{0}\times 10^{-13}  $ & $ 4.7\times 10^{29}$  &  $1.9\times 10^{-12}$  & $4.4\times 10^{30}$  &  $4.0\times 10^{-12}$ &  $9.4\times 10^{30}$  & 0.34      & 5, X	     \\  
\hline
\end{tabular}
\tablefoot {\tablefoottext{a}{Errors are given in parentheses.}
\tablefoottext{b}{In units of $10^{22}$~cm$^{-2}$.}
\tablefoottext{c} {Reference: {1: New analysis of Spitzer c2d sample, for original analysis see \citet{lahuis07}; 2: \citet{pascucci07}; 3: archival GTO/GO observations, see Najita \& Carr (in prep.);
                 4: \citet{herczeg07}; 5:~\mbox{\citet{boekel09}}; 6: \citet{espaillat07}; C: from {\it Chandra} archive; X: from {\it XMM-Newton} archive.}}   }           
\end{table}