Figure containing the power spectra used in this work. Top left: nonlinear matter auto-power spectrum P_mm (solid red line), the void auto-power spectrum P_vv without the shot noise (dashed blue line), computed assuming the pessimistic void bias scenario with b_v eff ≈ −11.9, and the absolute value of the void-matter cross-power spectrum P_vm (dot-dashed black line), all computed at redshift z = 0.001. Top right: tomographic void angular auto-power spectra for the diagonal (i = j) tomographic bins, without shot noise. Bottom left: tomographic lensing auto-power spectra for the diagonal (i = j) tomographic bins, without shape noise. Bottom right: tomographic void-lensing angular cross-spectra for the diagonal (i = j) tomographic bins. All the spectra are theoretically evaluated in the reference cosmology reported in Table 1 and the bin endpoints are given in Eq. (24).