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Fig. 9.


Measured RAR of isolated KiDS-bright lenses (black points with 1σ error bars) divided into four stellar mass bins. The mean galaxy mass (stars + cold gas) of the lenses is shown at the top of each panel. At increasing stellar mass, the measurements seem to rise above the predictions from MOND (grey solid line) and EG (red dashed line). However, at scales larger than (light blue shaded region) this could be caused by false positives in the isolated galaxy sample due to the KiDS-bright redshift uncertainty.

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