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Fig. 7.


Stellar mass histogram of the red (early-type) and blue (late-type) isolated KiDS-bright galaxies (red and blue lines), divided by u − r colour (mu − mr ≶ 2.5 mag). To isolate the effect of galaxy type on the RAR from that of M, we select two samples with the same stellar mass distribution by randomly removing galaxies from both samples until only the overlapping region (light blue shaded region) remains.

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