Accumulated fraction of mergers for type I (yellow), type II (blue), and type III (pink) disk galaxies across three stellar mass bins: ﹩\mathrm{log}({M}_{\star }/{M}_{\odot })=10.0﹩–10.4 (left), 10.4–10.8 (middle), and 10.8–11.2 (right). The fraction of galaxies experiencing at least one major merger (solid profiles, mass ratio >1:4) or minor merger (dashed profiles, mass ratio 1:4–1:10) as a function of look-back time.