Tidal response of TOI-5882 as a function of the dimensionless forcing frequency σ_m,k/Ω_orb, computed with GYRE-tides using α_frq scanning continuously to sample the forcing-frequency space. The blue and orange curves show the logarithmic amplitudes of the normalized radial displacement (﹩\mathrm{log}| {\tilde{\xi }}_{r}/R| ﹩) and luminosity perturbation (﹩\mathrm{log}| \delta \tilde{L}/L| ﹩), respectively, both evaluated at the stellar surface. Finally, gray points show the inverse normalized-mode inertia from a free-oscillation GYRE calculation spanning the same frequency range. We use the same stellar model as in Figure 2 to perform these calculations.