Fig. 1.
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Top: Halo mass function of N-cluster Run simulation. Bottom: Comparison with stellar mass function of the N-cluster Run simulation and other studies. The Orange solid and cyan dashed lines represent the simulation function from the N-cluster Run and the Illustris-TNG 100 simulation (Pillepich et al. 2018). Gray circles and blue triangles are observational function from SDSS (Bernardi et al. 2013) and DESI Y1 data (Wang et al. 2024).
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