Table 3: Overview of the $M_{\rm ap}$ 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 ( $80 \hbox {$^{\prime \prime }$ }$), 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).
  $\theta _{\rm out}$ N $\sigma _{\varepsilon }$ $\Delta \alpha [\hbox{$^{\prime\prime}$ }]$ $\Delta \delta [\hbox{$^{\prime\prime}$ }]$ $M_{\rm ap}$ SNR
$\vert\mbox{\boldmath${\rm\varepsilon}$\unboldmath }\vert < 0.8$, 80 $\hbox {$^{\prime \prime }$ }$ 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 $\hbox {$^{\prime \prime }$ }$ 560 0.39 20 26 0.030 2.2
all galaxies 120 $\hbox {$^{\prime \prime }$ }$ 907 0.39 0 0 0.025 2.4
  140 $\hbox {$^{\prime \prime }$ }$ 1188 0.38 -22 6 0.022 2.5
$\vert\mbox{\boldmath${\rm\varepsilon}$\unboldmath }\vert < 0.8$, 80 $\hbox {$^{\prime \prime }$ }$ 138 0.40 32 -32 0.060 2.1
$P^{\rm g}_s > 0.3$, 100 $\hbox {$^{\prime \prime }$ }$ 212 0.41 0 -18 0.060 2.7
weighted, 120 $\hbox {$^{\prime \prime }$ }$ 314 0.42 -12 -10 0.063 3.3
m > 26.5 140 $\hbox {$^{\prime \prime }$ }$ 392 0.42 -12 12 0.060 3.5
$\vert\mbox{\boldmath${\rm\varepsilon}$\unboldmath }\vert < 0.8$, 80 $\hbox {$^{\prime \prime }$ }$ 126 0.40 - - -0.034 -1.3
$P^{\rm g}_s > 0.3$, 100 $\hbox {$^{\prime \prime }$ }$ 204 0.40 - - -0.032 -1.5
weighted, 120 $\hbox {$^{\prime \prime }$ }$ 294 0.39 - - -0.014 -0.7
25.5 < m < 26.5 140 $\hbox {$^{\prime \prime }$ }$ 374 0.40 - - -0.008 -0.5
$\vert\mbox{\boldmath${\rm\varepsilon}$\unboldmath }\vert < 0.8$, 80 $\hbox {$^{\prime \prime }$ }$ 134 0.36 18 34 0.068 2.8
$P^{\rm g}_s > 0.3$, 100 $\hbox {$^{\prime \prime }$ }$ 220 0.36 4 16 0.045 2.4
weighted, 120 $\hbox {$^{\prime \prime }$ }$ 309 0.35 0 0 0.031 1.9
m < 25.5 140 $\hbox {$^{\prime \prime }$ }$ 402 0.35 - - 0.009 0.7

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