Multi-scale grid used for binning the shear measurements in the clean catalogue. The grid is centred on the cluster. Left: Number of galaxies per square arcminute in each bin when only considering galaxies in the tomographic bins 3–10 described in Schrabback et al. (2025). The smallest bins in the centre are approximately 1′ × 1′ while at the edges the bins are $2\stackrel{\prime }{.}24\times 2\stackrel{\prime }{.}24$. The full area is $26\stackrel{\prime }{.}85\times 26\stackrel{\prime }{.}85$. A similar grid configuration is adopted for the Gaussian functions in the distribution in mass. For the mass grid, the central 4′×4′ region (where the strong lensing constraints are found) is marked with a yellow square. This small region is further divided with an additional set of 123 smaller Gaussians (not shown). Middle and right: Observed shear γ₁ and γ₂ in the same multi-scale grid, same field of view, and for LensMC. The classic structure of γ₁ and γ₂ can be seen (i.e. horizontal and π/4-oriented quadrupole).