Fig. 5.
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Top: median (solid lines) and 16th–84th percentile region (shaded area) of the satellite velocity dispersion as a function of halo mass for a number density of nden = 0.0316 h3 Mpc−3. Results from the MTNG-DMO and MTNG simulations are shown in black and orange, respectively. Bottom: median (solid lines) and 16th–84th percentile region (shaded area) of the ratio of velocity dispersions between matched haloes in the MTNG and MTNG-DMO simulations, for the three number densities used in this work (as labelled).
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