\begin{table}%t1
\caption{\label{mags}Near-Infrared photometry of the PHL~5038 binary system and nearby calibration star.}
\small%\centerline
 {
\begin{tabular}{c c c c c c}        
\hline\hline  
Bandpass &      $\lambda$     &  PHL~5038 &       PHL~5038A  &    PHL~5038B    &          2MASS J22203205-0040210\\
         &      ($\mu$m)      &  (mag) &      (mag)      &    (mag)        &          (mag)\\
\hline
&&&&& \\[-8pt]
$Y^{1}$      &      1.03        & $16.89\pm0.01$ &   --   &   --     & -- \\
$J^{1}$      &      1.25        & $16.73\pm0.02$ &   --   &   --     & -- \\
$H^{1}$      &      1.63        & $16.44\pm0.03$ &   --   &   --     & -- \\
$K^{1}$      &      2.20        & $16.31\pm0.04$ &   --   &   --     & -- \\
$H^{2}$      &      1.65        &   --   &     $16.82\pm0.07$ & $17.84\pm0.08$    &      $14.447\pm0.053$\\
$K^{2}$      &      2.19        &   --   &     $16.72\pm0.07$ & $17.18\pm0.08$    &      $14.161\pm0.051$\\
\hline
\end{tabular}}
\medskip
$^{1}$ {\it UKIDSS} passbands as described in Hewett et~al. (\cite{hew06}).
$^{2}$~$H$- and $K$-band photometry were obtained on a single night.  The photometric errors were calculated using a 5\%~error from the nearby 2MASS star used for flux calibration, a~$2{-}3$\% photometric measurement error, and an assumed 5\% internal error typical of near-infrared arrays.  The final column displays the nearby 2MASS calibration star with its 2MASS catalogue
photometry and errors. Colour transformations between the filters are of the order of 1\% (Carpenter \cite{carp01}) and so are neglected.
\end{table}