Specific angular momentum of dark matter particles for the haloes studied. Top panel: computed it through Lagrangian-selection within the 5%R200 at z = 0. Therefore, we follow the same particles and compute the specific angular momentum for each redshift. We present our results for the SPH haloes (filled lines) and their DMO counterparts (dashed lines). We also include the halo Aq-C-M14 (solid grey line). Bottom panel: computed it through Eulerian-selection within the 5%R200, z as a function of redshift for the SPH haloes (filled lines) and their DMO counterparts (dashed lines). We also include the halo Aq-C-M14 (solid grey line).
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