Same as the bottom panels in Fig. 3 for four clusters at an increasing distance from us, from left to right, top to bottom. Although these clusters are less constrained, the agreement between observed and simulated waves is still visually good, especially for the first two. The dark matter halo masses in the simulation are M = 9.0 × 10¹⁴ M_⊙, M = 12.6 × 10¹⁴ M_⊙, M = 6.6 × 10¹⁴ M_⊙, and M = 11.7 × 10¹⁴ M_⊙ for Abell 569, Coma, Abell 85, and Abell 2256 cluster counterparts, respectively.