\begin{table}%t7
\caption{\label{prae_nir_phot}Near-infrared photometry of a few new Praesepe candidates.}
\small           
%\centerline
{
\begin{tabular}{llcccccc}
\hline    
\hline    
Object                                  & Teles. & $J$            & $H$            & $K_{\rm s}$          & $z'-J$        & $J-K_{\rm s}$       & Phot. Prob.$^{{a}}$ \\
\hline   \noalign{\smallskip} 
Prae~J083850.6$+$192317$^{{b}}$ & 2MASS  & 16.37~$\pm$~0.11 & 16.01~$\pm$~0.18 & 15.40~$\pm$~0.19 & 1.20~$\pm$~0.23 & 0.97~$\pm$~0.12 & high/high\\
Prae~J084051.2$+$191010$^{{c}}$ & 2MASS  & 16.75~$\pm$~0.15 & 15.76~$\pm$~0.15 & 15.59~$\pm$~0.23 & 1.00~$\pm$~0.25 & 1.16~$\pm$~0.27 & low/high\\
WFC~24$^{{d}}$                  & TCS    & 17.71~$\pm$~0.33 &                &                & 2.6~$\pm$~0.4   &               & high/high\\
Prae~J084111.9$+$192043                & WHT    & 19.85~$\pm$~0.07 & 18.95~$\pm$~0.11 & 18.28~$\pm$~0.10 & 2.48~$\pm$~0.21 & 1.57~$\pm$~0.12 & high/high\\
\hline    
\end{tabular}}
\smallskip
$^{{a}}$ Optical / near-infrared photometric cluster membership probability;
$^{{b}}$ 2MASS~J08385059$+$1923164;
$^{{c}}$ 2MASS~J08405122$+$1910106;
$^{{d}}$~\mbox{$J = 17.99 \pm0.03$}, $H = 17.30  \pm0.02$, $K = 16.78 \pm0.02$ (Chappelle et~al. \cite{chappelle05}).
\end{table}