\begin{table}%T12
\caption{Probable late-type cluster members based on proper motion
(Platais et~al. \cite{PKB}) that were not detected in X-rays.\label{upperlimits} }
%%%%\centerline


\par
{
\begin{tabular}{rccccl}
\hline\hline
Platais\# & $V$ & $B-V$ & log~$L_{\rm x}$ & log~$\frac{L_{\rm x}}{L_{\rm bol}}$&
Notes \\
\hline
 987 & 13.51 & 1.12 & $<$28.55 & $<$--4.33 & \\
1238 & 12.75 & 0.68 &    --    & $<$--4.63 & * \\
1315 & 12.30 & 0.81 & $<$28.95 & $<$--4.27 & \\
1574 & 14.13 & 1.17 & $<$29.11 & $<$--3.57 & \\
2223 & 11.04 & 0.59 & $<$28.53 & $<$--5.15 & \\
% 2381 & 11.86 & 0.73 &    29.16 &    --4.22 & * \\
2767 & 12.11 & 0.95 & $<$28.76 & $<$--4.59 & \\
3678 & 11.49 & 0.67 & $<$28.50 & $<$--5.01 & \\
6567 & 13.46 & 1.23 & & & * \\
6783 & 14.17 & 0.67 &    --    & $<$--3.74 & * \\
6819 & 13.42 & 0.88 &    --    & $<$--4.48 & * \\
8409 & 13.39 & 1.06 & $<$28.83 & $<$--4.09 & \\
8422 & 13.04 & 1.01 & $<$29.08 & $<$--3.92 & \\ 
\hline
\end{tabular}}
\par
\medskip
Notes:\\ 
\#1238: photometry suggests membership of cluster B.\\
\#6567: no X-ray upper limit because too close to X177.\\
\#6783: photometry suggests non-membership.\\
\#6819: photometry suggests membership of cluster B.  
\end{table}