\begin{table}%t1
\caption{\label{t:phot}Observed magnitudes and fluxes for the presumed
infrared/optical  pulsar/PWN counterpart of J1124-5916, and de-reddened fluxes for the $A_V$ range of 1.86--2.10.}
%\centerline
 {\small \begin{tabular}{llll}
\hline\hline
$\lambda_{\rm eff}$(band)  & Mag.  &  $\log$ Flux & $\log$ Flux\\
&  observed$^a$ &  observed$^a$ &  de-reddened$^a$ \\
($\mu$m) & (mag) & ($\mu$J) & ($\mu$J)    \\
\hline
&Infrared & Spitzer  &   \\[1mm]
70  & $\ga$6.8  &$\la$3.2 &$\la$3.2   \\[1mm]
 24 &  $\ga$10.2  &$\la$2.8 &$\la$2.85    \\[1mm]
 8.0                               & 14.2(3)                           &2.13(16)                                    & $\rm 2.18(^{+16}_{-17})$    \\[1mm]
 4.5                              & 15.9(4)                            &1.90(21)                                    &  $\rm 1.95(^{+21}_{-22})$  \\[1mm]
 \hline
&  Optical                                 &                     VLT                  &                                 \\
%\hline
 0.77($I$)                   & 23.12(13)                      & 0.13(5)                                        &  $\rm 0.66(^{+6}_{-10})$    \\[1mm]
 0.66($R$)                  & 24.12(13)                    & $-$0.17(5)                                       &  $\rm 0.51(^{+7}_{{-12}})$         \\[1mm]
 0.55($V$)                 & 24.29(13)                    & $-$0.16(5)                                        & $\rm 0.66(^{+7}_{-13})$          \\[1mm]
\hline
\end{tabular}}
\medskip
$^a$~Numbers in brackets are 1$\sigma$ uncertainties referring to last significant digits quoted.
\end{table}