\begin{table}%ta1
      \caption{New probable cluster non-members.} 
         \label{interesting}
     $$ 
       \small  \begin{tabular}{lccccccr}
            \hline
            \hline
            \noalign{\smallskip}
Id.     & $\alpha^{J2000}$ & $\delta^{J2000}$ & $I \pm \delta I$ (mag) &  $J \pm
\delta J$ (mag) &  $H \pm \delta H$ (mag) &  $K_{\rm s} \pm \delta K_{\rm s}$ (mag)
& Remarks  \\
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
1       & 05 39 25.4    & --02 29 43    & 23.11~$\pm$~0.18        & 20.08~$\pm$~0.10    
   & 19.43~$\pm$~0.07        & 19.07~$\pm$~0.07 & Early L-type field dwarf?    \\      
2       & 05 38 44.6    & --02 44 40    & 23.8~$\pm$~0.5          & 20.64~$\pm$~0.08    
   & 19.90~$\pm$~0.09        & 19.22~$\pm$~0.10 & Late L-type field dwarf?     \\      
3       & 05 39 59.3    & --02 52 56    & 23.3~$\pm$~0.3          & 20.82~$\pm$~0.09    
   & 19.6~$\pm$~0.2          & 18.65~$\pm$~0.07 & Radio galaxy?                \\      
4       & 05 40 04.7    & --02 29 27    & $\gtrsim$24.5         & 21.56~$\pm$~0.10    
   & 20.01~$\pm$~0.12        & 18.52~$\pm$~0.13 & Extremely red galaxy?        \\      
            \noalign{\smallskip}
            \hline
         \end{tabular}
     $$ 
   \end{table}