tSZ and kSZ power spectra up to r_max = 110 Mpc from several hydrodynamical simulations. As in Fig. 8, the solid red line and the orange and green areas are determined from the SLOW simulation, and the dashed lines are the corresponding predictions from the halo model. The solid purple lines are estimated from local Universe maps determined from the Coruscant simulation, and the gray areas are 90% percentiles from the Magneticum simulation.