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Fig. 10.


Measured RAR of KiDS-bright lenses (points with 1σ error bars), respectively for isolated dwarfs (, blue) and the full isolated galaxy sample (, black). Due to the low S/N of the dwarf lensing signal, the number of gbar-bins is reduced from 15 to 5. We find that the RAR of dwarfs is consistent with that of our regular sample, and with the extrapolated MOND and EG predictions (grey solid and red dashed lines), which are shown as a reference.

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