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Fig. A.1.

image

Mass-density MGE for FCC 153. Top: contours of the projected mass density (black), the mass density MGE (red), and the surface brightness MGEμ (blue). Bottom: ratio between the mass and surface-brightness models, showing the structural differences. This panel is normalised by the average M/L such that values of 1.0 (white) are consistent with the assumption of a spatially-constant M/L, and any deviations are percentages in stellar mass. The outline of the MUSE mosaic is shown in dashed brown.

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