Fig. 9.

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Stellar mass function at z = 0. In each run, we consider the stellar mass measured within r = 30 kpc from the halo centre and qualitatively compare it to observations from SDSS (Bernardi et al. 2013) and GAMA (Wright et al. 2017). Solid and dashed lines represent the 100/A and 50/A runs, while we show the 50/B measurements (dot-dashed) only for the WDM1 scenarios. The colour scheme of the different dark matter models is the same as in Fig. 6.
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