\begin{table}%t3
\caption{Overview of the $\map$ values and signal-to-noise ratios of
  the peaks found in the analyses of the HST~data.
  We also give the number of galaxies located
  in the aperture~($N$), and the (weighted) average galaxy ellipticity~$\sigma_{\varepsilon}$, as well as the offset to the assumed centroid position, measured in the
  sky coordinate system. For the smallest filter scale~($80 \arcsec$), the anlysis of all galaxies yields two peaks in the vicinity of the dark clump position, both of which are listed. For the medium bright
  bin, there is no peak close to the dark clump in the largest two~filter
  scales~-- we then quote the values at the reference position (in italics).}\label{tab:hst-map-results}
%\centering
\small
\begin{tabular}{l|rcccccc}
\hline \hline
% &&&&&&&  \\[-8pt]
& $\theta_{\rm out}$ & $N$ & $\sigma_{\varepsilon}$ & $\Delta \alpha [\arcsec]$ & $\Delta \delta
[\arcsec]$ & $\map$ & {\it SNR} \\
% &&&&&&&  \\[-8pt]
\hline
$|\bfmath{\varepsilon}| < 0.8$, &  80$\arcsec$ & 352 & 0.39 & 34 & 32 & 0.037 & 2.2 \\
$P^{\rm g}_s > 0.3$,&              & 410 & 0.38 &  $-42$ &  $-52$ & 0.033 & 2.3 \\
weighted,           & 100$\arcsec$ & 560 & 0.39 &  20 &  26 & 0.030 & 2.2 \\
all galaxies        & 120$\arcsec$ & 907 & 0.39 &  0 &  0 & 0.025 & 2.4 \\
                    & 140$\arcsec$ & 1188 & 0.38 & $-22$ &   6 & 0.022 & 2.5 \\
\hline
$|\bfmath{\varepsilon}| < 0.8$, &  80$\arcsec$ & 138 & 0.40 &  32 & $-32$ & 0.060 & 2.1 \\
$P^{\rm g}_s > 0.3$,&   100$\arcsec$ & 212 & 0.41 &  0 &  $-18$ & 0.060 & 2.7 \\ 
weighted,           & 120$\arcsec$ & 314 & 0.42 &  $-12$ &  $-10$ & 0.063 & 3.3 \\
$m > 26.5$         & 140$\arcsec$ & 392 & 0.42 &  $-12$ &  12 & 0.060 & 3.5 \\
\hline
$|\bfmath{\varepsilon}| < 0.8$, & 80$\arcsec$ & \textit{126} & \textit{0.40} & $-$ & $-$ & \textit{$-$0.034} & \textit{$-$1.3} \\
$P^{\rm g}_s > 0.3$,& 100$\arcsec$ & \textit{204} & \textit{0.40} & $-$ & $-$ & \textit{$-$0.032} & \textit{$-$1.5} \\
weighted,           & 120$\arcsec$ & \textit{294} & \textit{0.39} & $-$ & $-$ & \textit{$-$0.014} & \textit{$-$0.7} \\
$25.5 < m < 26.5$ & 140$\arcsec$ & \textit{374} & \textit{0.40} & $-$ & $-$ & \textit{$-$0.008} & \textit{$-$0.5} \\
\hline
$|\bfmath{\varepsilon}| < 0.8$, & 80$\arcsec$ & 134 & 0.36 &  18 &  34 & 0.068 & 2.8 \\
$P^{\rm g}_s > 0.3$,             & 100$\arcsec$ & 220 & 0.36 &   4 &  16 & 0.045 & 2.4 \\
weighted,                      &  120$\arcsec$ & 309 & 0.35 &   0 &   0 & 0.031 & 1.9 \\
$m < 25.5$ & 140$\arcsec$ & \textit{402} & \textit{0.35} & $-$ & $-$ & \textit{0.009} & \textit{0.7} \\
\hline
\end{tabular}
\end{table}