Density of satellite galaxies as a function of distance from the halo centre for the n_den = 0.0316 h³ Mpc⁻³ sample. The left, middle, and right panels show density profiles for halo masses of 10^13.5, 10¹⁴, and 10^14.5 h⁻¹ M_⊙, respectively. Black lines represent results from the MTNG-DMO simulation, while orange lines correspond to the hydrodynamic MTNG simulation. The vertical dashed lines represent the value of one virial radius r_200c.