\begin{table}%t1
\caption{\label{tab1}Flux densities measured from the MIPS and {\it Herschel} maps.  }
%\centering
\par
\begin{tabular}{llllllllll}
\hline \hline \noalign{\smallskip}
ID & RA & Dec & Flux$_{24}$ & Flux$_{100}$ & Flux$_{160}$ & Flux$_{250}$ & Flux$_{350}$ & Flux$_{500}$ \\
   &[deg] & [deg] & [mJy] & [mJy] & [mJy] & [mJy] & [mJy] & [mJy]\\
\hline \noalign{\smallskip}
HLS01 &  104.72828 &  --55.88917 &      0.40  $\pm$  0.01 &    $ \ldots$  &    $ \ldots$  &       21.1 $\pm$    2.5 &       10.0 $\pm$    3.5 &    $<$$7.8$\tablefootmark{b} \\
HLS02 &  104.46419 &  --56.02209 &      0.15 $\pm$  0.01 &    $ \ldots$  &    $ \ldots$  &       10.1 $\pm$    2.4 &       16.2 $\pm$    3.5 &       14.4 $\pm$    4.0\\
HLS03 &  104.48783 &  --56.03070 &      0.39 $\pm$  0.02 &    $ \ldots$  &    $ \ldots$  &        9.0 $\pm$    2.4 &        9.5 $\pm$    3.4 &    $<$$7.8$\tablefootmark{b} \\
HLS04 &  104.45727 &  --55.91533 &      0.39 $\pm$  0.01 &    $ \ldots$  &    $ \ldots$  &       18.6 $\pm$    2.8 &       13.2 $\pm$    3.6 &    $<$$7.8$\tablefootmark{b} \\
HLS05 &  104.60260 &  --55.92013 &      0.71 $\pm$  0.02 &       75.4 $\pm$    1.3 &      164.4 $\pm$    5.1 &      168.9 $\pm$    6.2 &      120.0 $\pm$    4.1 &       58.4 $\pm$    4.4\\
HLS06 &  104.64300 &  --55.90990 &      0.40 $\pm$  0.01 &        9.9 $\pm$    1.2 &       28.4 $\pm$    2.4 &       44.6 $\pm$    2.8 &       39.0 $\pm$    3.5 &       25.2 $\pm$    4.0\\
HLS07 &  104.60545 &  --55.89051 &      0.29 $\pm$  0.01 &        7.0 $\pm$    1.3 &        7.8 $\pm$    2.1 &        8.2 $\pm$    2.8 &    $<$$8.4$\tablefootmark{b}  &    $<$$7.8$\tablefootmark{b} \\
HLS08 &  104.63628 &  --55.98351 &      0.135 $\pm$  0.003 &        2.7 $\pm$    1.1 &        4.6 $\pm$    2.1 &    $<$$6.0$\tablefootmark{b}  &    $<$$8.4$\tablefootmark{b}   &    $<$$7.8$\tablefootmark{b} \\
HLS09 &  104.55591 &  --55.87279 &      0.65 $\pm$  0.02 &    $ \ldots$  &    $ \ldots$  &       23.2 $\pm$    2.6 &       12.9 $\pm$    3.5 &    $<$$7.8$\tablefootmark{b} \\
HLS10 &  104.54350 &  --55.98005 &      0.53 $\pm$  0.02 &       16.7 $\pm$    1.4 &       22.6 $\pm$    2.1 &       13.9 $\pm$    2.4 &    $<$$8.4$\tablefootmark{b}  &    $<$$7.8$\tablefootmark{b} \\
HLS11 &  104.56008 &  --55.95848 &      0.47 $\pm$  0.01 &        7.4 $\pm$    1.1 &       15.1 $\pm$    2.1 &       33.1 $\pm$    2.7 &       36.9 $\pm$    3.5 &       18.8 $\pm$    4.1\\
HLS12 &  104.62997 &  --55.94386 &      0.046 $\pm$  0.003 &    $<$$2.4$\tablefootmark{b}  &        4.3 $\pm$    2.1 &        7.8 $\pm$    2.5 &       11.4 $\pm$    3.4 &    $<$$7.8$\tablefootmark{b} \\
HLS13 &  104.60567 &  --55.94490 &      0.28 $\pm$  0.01 &        2.9 $\pm$    1.1 &        5.5 $\pm$    2.0 &       10.1 $\pm$    2.5 &       19.6 $\pm$    3.5 &    $<$$7.8$\tablefootmark{b} \\
HLS14 &  104.64689 &  --55.88658 &      0.136 $\pm$  0.004 &        3.0 $\pm$    1.2 &        4.4 $\pm$    2.1 &    $<$$6.0$\tablefootmark{b}  &    $<$$8.4$\tablefootmark{b}  &    $<$$7.8$\tablefootmark{b} \\
HLS15 &  104.73730 &  --55.88516 &      0.16 $\pm$  0.02 &    $ \ldots$  &    $ \ldots$  &       11.1 $\pm$    2.7 &       15.3 $\pm$    3.8 &       11.7 $\pm$    3.7\\
HLS16 &  104.58575 &  --55.93920 &      0.83 $\pm$  0.02 &       25.3 $\pm$    1.3 &       51.3 $\pm$    2.5 &       47.7 $\pm$    2.6 &       24.0 $\pm$    3.6 &       10.2 $\pm$    3.7\\
HLS17 &  104.64463 &  --56.00850 &      0.71 $\pm$  0.02 &       24.7 $\pm$    1.2 &       56.5 $\pm$    3.4 &       49.2 $\pm$    3.4 &       35.5 $\pm$    3.7 &       17.9 $\pm$    3.7\\
HLS18$_{A}$\tablefootmark{a} &  104.65471 &  --55.95193 &      0.49 $\pm$  0.01 &        7.0 $\pm$    1.2 &       24.5 $\pm$    2.1 &       65.3 $\pm$    2.8 &       98.6 $\pm$    3.9 &      101.4 $\pm$    4.0\\
HLS18$_{B}$\tablefootmark{a} &  104.65861 &  --55.95057 &        0.36 $\pm$  0.01 &      3.8 $\pm$  1.1   &       14.0 $\pm$    2.5 &        $<$$6.0$\tablefootmark{b}        &    $<$$8.4$\tablefootmark{b}            &    $<$$7.8$\tablefootmark{b}\\
\par
HLS19 &  104.59877 &  --55.87833 &      1.10 $\pm$  0.03 &    $ \ldots$  &    $ \ldots$  &       40.9 $\pm$    2.9 &       21.6 $\pm$    4.0 &        9.4 $\pm$    3.7\\
\hline
\end{tabular}
\tablefoot {{The 500~$\mu$m map was corrected for SZ contamination before extracting the photometry. These measurements have not been corrected for the amplification due to gravitational lensing.}  \tablefoottext{a}{Multiple images of the highly lensed galaxy \citep{Gonzalez2009};}
\tablefoottext{b}{upper limits correspond to statistical 3-$\sigma$ noise levels of each map.}}
\end{table}