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Fig. 2.


Comparison of the spherically averaged dark matter profiles from the SPH run at z ∼ 0 with the fits of Einasto profile (green dotted lines) and Di Cintio et al. (2014a; DC14) profile. In the case of DC14, we adopted two methods: the first assumes the concentration parameter DMO as a free parameter (named as DC14 fitI, blue dashed lines); and the second method considers both the concentration parameter and the halo mass as free parameters (named as DC14 fitII, dashed purple line). The grey dashed lines in profiles Aq-C-SPH and Aq-E-SPH5 represent three times the gravitational softening for these haloes. We also include the rms for each fit in the lower panels.

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