Aperture mass maps of 1 deg² obtained from the full redshift distribution (0 <  z_all <  3), for five continuous redshift slices (0 <  z₁ <  0.4676, 0.4676 <  z₂ <  0.7194, 0.7194 <  z₃ <  0.9625, 0.9625 <  z₄ <  1.3319, 1.3319 <  z₅ <  3) and for a few cross-combinations of redshift slices (z₂ ∪ z₃, z₂ ∪ z₄, z₂ ∪ z₃ ∪ z₄). Massive foreground halos are traced in multiple redshift planes while the noise fluctuates randomly. The cross-M_ap terms allow us to retain the information about correlations of structures in between slices.