\begin{table}%t1
\caption{Properties of discless high-velocity stars in the ONC.}\label{tab:obs_highvel}
\small
  %\centerline
{
\begin{tabular}{l*{13}{r}l}
\hline\hline\noalign{\smallskip}
ID$^a$
& $r$$^b$
& $\mu_x$$^c$
& $\sigma_x$ 
& $\mu_y$ 
& $\sigma_x$ 
& $P$$^d$
& $J$$^e$
& $H$
& $K$
& $L$
& SpT$^f$
& $m$$^g$
& $\log{t}$$^h$
& excess$^i$ \\
$\rm \left[JW\right]$            & $\rm\left[pc\right]$  & $\rm\left[km~s^{-1}\right]$  & $\rm\left[km~s^{-1}\right]$      & $\rm\left[km~s^{-1}\right]$  & $\rm\left[km~s^{-1}\right]$     & $\rm\left[\%\right]$ & $\rm\left[mag\right]$ & $\rm\left[mag\right]$ & $\rm\left[mag\right]$ & $\rm\left[mag\right]$ &       & $\rm\left[{\it M}_\odot\right]$ & $\rm\left[yr\right]$             \\
\hline
\object{JW 19}    & 1.99  & --12.2   &   4.2       &   0.2   &   2.2      & 84   & 12.98 & 12.26 & 11.87 &       & M5.5  & 0.16    & 4.05      & no    \\
\object{JW 45}    & 1.12  & --13.0   &   0.6       &  --0.8   &   0.8      &  0   &  8.83 &  8.28 &  8.05 &  7.89 & K3    & 0.94    & 4.52      & no    \\
\object{JW 505}   & 0.10  &  --4.2   &  11.4       & --22.8   &   8.8      & 93   & 12.33 & 11.65 & 11.18 & 10.65 & M2    & 0.20    & 4.21      & ?     \\
\object{JW 510}   & 0.36  &  --5.0   &   2.8       &   8.8   &   2.4      & 95   & 13.01 & 12.18 & 11.76 & 11.16 & M5    & 0.14    & 4.77      & yes   \\
\object{JW 559}   & 0.19  & --11.6   &   3.2       &   9.8   &   3.8      & 99   & 12.43 & 11.74 & 11.30 & 11.04 & M5.5e & 0.16    & 3.97      & no    \\
\object{JW 569}   & 0.24  & --12.0   &   3.8       &  -3.6   &   3.4      & 92   & 12.47 & 11.58 & 11.00 & 10.14 & M3.5  & 0.09    & 3.11      & yes   \\
\object{JW 616}   & 0.30  &   9.4   &   5.6       &   9.0   &   2.8      & 95   & 13.21 & 12.36 & 11.91 & 11.50 & M3.5  & 0.15    & 4.24      & no    \\
\hline
\end{tabular}}
\medskip
$^a$ Stellar ID from \citet{1988AJ.....95.1755J}.
$^b$ Projected distance from   {$\theta^1{\rm{C}}\:{\rm{Ori}}$}.
$^c$ Proper motion and associated error.
$^d$  Probability of cluster membership.
$^e$ Apparent magnitude in specified band filter.
$^f$ Spectral type.
$^g$ Stellar mass.
$^h$ Stellar age.
$^i$ Detection of excess emission.
\end{table}