\begin{table}%t2
\caption{\label{tab:mags}The derived apparent magnitudes for \epsba, Bb.}
\small%\centerline
 {
\begin{tabular}{lll}
\hline
\hline\noalign{\smallskip}
Passband &  Ba         & Bb                 \\
\hline	
$V$     & 24.12 $\pm$ 0.03    & $\geq$26.60$\pm$ 0.05 \\
$R$     & 20.65 $\pm$ 0.01    & 22.35 $\pm$ 0.02 \\
$I$     & 17.15 $\pm$ 0.02    & 18.91 $\pm$ 0.02 \\
$z$     & 15.07 $\pm$ 0.02    & 16.53 $\pm$ 0.02 \\
$J$     & 12.20 $\pm$ 0.03    & 12.96 $\pm$ 0.03 \\
$H$     & 11.60 $\pm$ 0.02    & 13.40 $\pm$ 0.03 \\
$K$     & 11.42 $\pm$ 0.02    & 13.64 $\pm$ 0.02 \\
$L'$    & \ \ 9.71 $\pm$ 0.06 & 11.33 $\pm$ 0.06 \\
$M'$    & 10.67 $\pm$ 0.23    & 11.04 $\pm$ 0.23 \\
\hline		
\end{tabular}}
\medskip
The optical magnitudes are in the FORS2 system as described in Appendix~\ref{sec:phot_calib}, and the near-IR~magnitudes have been transformed into the MKO $\it JHKL'M'$~filters via synthetic photometry. The uncertainties for both objects are dominated by the uncertainties on the measured flux ratio and the standard star magnitudes. Absolute magnitudes may be derived using the distance
modulus of~$-2.205$.
\end{table}