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Fig. 1.


Stellar mass to halo mass relation for the five haloes studied: Aq-A-SPH (stars), Aq-C-SPH (triangles up), Aq-D-SPH (circles), Aq-E-SPH (squares) and Aq-C-M14 (triangles down). The results for the five haloes are plotted where colour code represents the different redshifts (z = 0 red, z = 1 green, z = 2 blue, z = 3 purple, and z = 4 orange). We follow the evolution of the SPH haloes with dotted lines. The grey filled line connects the different refshifts for Aq-C-M14. We compared our findings with the results of abundance matching technique from Guo et al. (2010), Behroozi et al. (2018), and Moster et al. (2018; see labels in the figure).

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