\begin{table}%t4
\par
\protect\caption{\label{LTcan}Coordinates and photometry of the new L- and T-type cluster member candidates$^a$.}
     {\footnotesize	
%\centerline
 {     \begin{tabular}{c c c c c c c c c c}
     	 \hline\hline
	 Name &
	 $\alpha$~~~~~~~~~~~~~~~~~~~~~~~~~$\delta$ &
	 $I$ &
	 $Z$ &
	 $J$ &
	 $H$ &
	 $K_{\rm s}$ &
	 $[3.6]$ &
	 $[4.5]$ &
	 $[5.8]$
         \\
	 & (J2000)~~~~~~~~~~(J2000) & (mag) & (mag) & (mag) & (mag) & (mag) & (mag) & (mag) & (mag)
	 \\
	 \hline
         \object{S~Ori~72} & 5 38 59.17 $-$2 35 26.0 & $>$24.1      & $>$23.3 & 20.89~$\pm$~0.06 & 19.57~$\pm$~0.03 & 18.72~$\pm$~0.05 & 17.65~$\pm$~0.11 & 17.51~$\pm$~0.29  & 17.28~$\pm$~0.38 \\
         \object{S~Ori~73} & 5 38 14.49 $-$2 45 11.8 & $>$24.5 & 23.5~$\pm$~0.5 & 20.91~$\pm$~0.07 & 20.83~$\pm$~0.12 & 20.91~$\pm$~0.15 & 19.64~$\pm$~0.35 & 18.77~$\pm$~0.35  & $>$16.0        \\
         \object{S~Ori~74} & 5 38 44.27 $-$2 40 07.9 & 24.6~$\pm$~0.4 & $>$23.3 & 21.1~$\pm$~0.1   & $>$18.54$^{b}$ & 19.38~$\pm$~0.10 & ...$^{c}$	   & ...$^{c}$       & $>$16.0        \\
	\hline
      \end{tabular}}
\par
\smallskip
$^a$ All have $[8.0]>15.1$~mag.
$^b$ Lower magnitude limit computed for the UKIDSS GCS specific field.
$^c$ Blended with a spike from the star \object{Mayrit~260182} (located at 11.8~arcsec).
      }
\normalsize
\end{table}