\begin{table}%t6
\caption{\label{tab:cands}The candidate list of the WFILAS survey after the selection
  as described in Sect.~\ref{sec:selection}. From left to right are
  the object name, the $B$, $R$, \med, \na, \nb\ and \nc\
  \mbox{$AB$-magnitudes}, line flux calculated from the narrowband
  magnitude in which the object was detected and line luminosity. For
  all measurements less than $2\sigma$ the $2\sigma$ upper limit has
  been given.}
%\centerline
{\begin{tabular}{rlcccccccc}
\hline\hline
\sext\ ID& Object ID                   & $B$                 & $R$                 & \med\            & \na\                & \nb\                & \nc\                & Line flux                & Luminosity  \\
         &                             &                     &                     &                  &                     &                     &                     & (10$^{-17}$~\lineunits) & (10$^{43}$~\ergs) \\
\hline
CDFS\_1864$^a$ & J033215.14-280013.9 & $>$26.25        & $>$26.56        & 24.72 $\pm$ 0.46 & 23.14 $\pm$ 0.26 & $>$24.27        & $>$23.93        &  6.5 $\pm$ 1.5 & 2.3 $\pm$ 0.5\\
CDFS\_4928$^a$ & J033145.97-275316.4 & $>$26.25        & $>$26.56        & 24.59 $\pm$ 0.41 & 23.38 $\pm$ 0.32 & 24.11 $\pm$ 0.47 & 23.61 $\pm$ 0.41 &  5.2 $\pm$ 1.6 & 1.8 $\pm$ 0.5\\
CDFS\_5388$^a$ & J033202.37-275211.3 & $>$26.25        & $>$26.56        & 24.70 $\pm$ 0.45 & 23.32 $\pm$ 0.31 & $>$24.27        & $>$23.93        &  5.5 $\pm$ 1.5 & 1.9 $\pm$ 0.5\\
 S11\_5236$^a~^b$ & J114334.98-014433.7 & $>$26.63        & $>$26.59        & 24.31 $\pm$ 0.42 & $>$24.13        & 23.05 $\pm$ 0.18 & $>$23.74        &  7.0 $\pm$ 1.2 & 2.5 $\pm$ 0.4\\
 S11\_8921$^c$ & J114218.90-013544.6 & $>$26.63        & 26.38 $\pm$ 0.45 & 23.88 $\pm$ 0.28 & 23.98 $\pm$ 0.47 & 23.41 $\pm$ 0.26 & $>$23.75        &  5.0 $\pm$ 1.2 & 1.8 $\pm$ 0.4\\
S11\_10595 & J114312.46-013049.6 & $>$26.63        & $>$26.60        & 24.44 $\pm$ 0.47 & $>$24.13        & 23.52 $\pm$ 0.28 & $>$23.75        &  4.5 $\pm$ 1.2 & 1.6 $\pm$ 0.4\\
 SGP\_8884$^d$ & J004525.38-292402.8 & $>$26.07        & $>$26.41        & 23.33 $\pm$ 0.20 & 22.73 $\pm$ 0.16 &                  & $>$24.06        &  9.5 $\pm$ 1.4 & 3.3 $\pm$ 0.5\\
\hline
\end{tabular}
 }
 \medskip
$^a$ {Galaxy is in the complete sample.}
$^b$ {Confirmed LAE at $z = 5.721$. See text and
  \citet{Westra05} for details.}
$^c$ {Signal-to-noise in the range $2{-}3\sigma$ for $R$ band
  in the 10 pixel aperture, but ${<}2\sigma$ in the 6 pixel aperture.}
$^d$ {Confirmed LAE at $z$ = 5.652. See text for details.}
\end{table}