Notes. The table shows the simulation name, the mass M_⋆, the average emitted luminosity L_⋆, the average approximate stellar radius R_⋆ (we note that the radii vary by about 20% during one pulsation period), effective temperature T_eff, surface gravity logg, the pulsation period P_puls, the half of the distribution of the pulsation frequencies σ_puls, and the stellar time t_avg used for the averaging of the rest of the quantities. All these quantities are from Freytag et al. (2017). The last four columns are the time-averaged value of the photocentre displacement ⟨P⟩=⟨(P_x² + P_y²)^(1/2)⟩, its standard deviation (σ_P), and the time-average of P_x and P_y.