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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