Comparison between ODLC in first approach and SDLCs for all scenarios in Figure 2. After generating 10⁵ SDLCs from each pair of maps, we show the best-fit SDLC (minimum RMS; left panels) and ten randomly chosen SDLCs that are characterised by RMS < 2.60 (out of a total of n; right panels). Each row corresponds to the same row position in Figure 2, so the results for the standard scenario without PBHs are depicted in the first row from the top (RMS_min = 1.67 and n = 10 919), and those for the non-standard scenarios are shown in successive rows: 45% of the mass in Jupiter-mass PBHs (RMS_min = 1.60 and n = 1536; second row), 81% of the mass in ∼0.1 M_⊙ PBHs (RMS_min = 1.68 and n = 152; third row), and 45% of the mass in ∼10 M_⊙ PBHs (RMS_min = 1.69 and n = 13 381; fourth row).