\begin{table}%T1
\par
\caption{\label{table1}{\it VRIJHK}s photometry of \#1916. 
Near-IR magnitudes are measured within 
1.5~arcsec apertures on seeing matched images. 
Limiting magnitudes in the visible bands correspond to a 
detection limit of~$1~\sigma$ within the near-IR reference seeing
aperture, which is equivalent to a 3$~\sigma$~detection on~4~ISAAC pixels.
Table entries denote the filter name (Col.~1), effective wavelength~(2), total 
exposure time~(3), the image quality/seeing~(4), and the observed 
magnitudes in the Vega~(5) and AB~(6)~systems.}
%\centering
\par
\begin{tabular}{lllllll}
\hline
\hline
Filter & $\lambda_{\rm eff}$ & $t_{\rm exp}$ & Seeing & mag    & mag   \\
       &   [$\mu$m]          & [ks]    & [$''$]    & [Vega] &  [AB] \\
\hline 
$V$       &0.54   &3.75   &0.76   &$>$28.5               &$>$28.6       \\
$R$       &0.66   &5.4    &0.69   &$>$28.5               &$>$28.7       \\
$I$       &0.81   &4.5    &0.78   &$>$27.6               &$>$28.1       \\
$J$       &1.26   &6.48   &0.65   &25.83 $\pm$ 1.00       &26.77 $\pm$ 1.00\\
$H$       &1.65   &13.86  &0.5    &23.59 $\pm$ 0.25       &25.00 $\pm$ 0.25\\
$K$s      &2.16   &18.99  &0.38   &23.64 $\pm$ 0.36       &25.51 $\pm$ 0.36\\
\hline
\end{tabular}
\end{table}