\begin{table}%t3
%\centering
\par
\caption { {Johnson-Cousins {\it BVRI}  and 2MASS {\it JHK}  photometry and derived
  photometric parallaxes based on HEN04. All "$r$'' band magnitudes are taken
  from the literature; objects labeled with an "*''
  have {\it BVI} photometry taken from the literature as described in 
  Sect.~2; other {\it BVI} magnitudes are found from in-house photometry. \label{photo}} }
\begin{tabular}{lcccccccr}%rrrrrrrrrrr}%lllllllll}
\hline  \hline
LHS &  $B$ &  $V$  &  $R$  &   $I$  &   $J$ & $ H$  &  $K$  & $\pi_{\rm P}$ \\          %   
\hline  \\	            							     %				     
\object{LHS~269} &18.16&16.80&14.76& 12.65&10.906 & 10.310 &  9.958 &$43.6\pm6.8$\\%	 
\object{LHS~279} &16.59&15.95&14.66& 12.76&11.333 & 10.842 & 10.609 &$17.6\pm2.7$\\%	 
\object{LHS~306} &16.10&14.52&12.58& 10.94& 9.359 &  8.764 &  8.497 &$72.9\pm10.$\\%	 
\object{LHS~318}*&16.10&15.51& --  & 13.00&12.503 & 11.983 & 11.797 &$ 5.6\pm1.2$\\%	 
\object{LHS~326}*&15.80&14.53& --  & 13.00&11.927 & 11.430 & 11.234 &$ 5.6\pm1.0$\\%	 
\object{LHS~334} &19.70&17.69& --  & 15.01&13.746 & 13.252 & 13.044 &$ 4.8\pm0.8$\\%	 
\object{LHS~356}*&17.20&16.37& --  & 13.00&13.307 & 12.877 & 12.621 &$ 4.7\pm1.2$\\%	 
\object{LHS~360} &16.00&15.28&14.28& 13.36&12.390 & 11.849 & 11.662 &$ 5.1\pm0.8$\\%	 
\object{LHS~370} &17.20&16.17&14.67& 12.85&11.054 & 10.553 & 10.254 &$30.4\pm4.6$\\
 \hline 					
\end{tabular}
\end{table}