“…We calculated the terminal Cretaceous disparity patterns of every dinosaur subgroup that is represented by a reasonable number of Campanian-Maastrichtian specimens that could be scored for large matrices of discrete characters. Analysed clades include: non-avian coelurosaurian theropods 28 , tyrannosauroid theropods 29 , pachycephalosaurs 30 , ceratopsids (most of which are chasmosaurines, because there is no available global phylogeny of ceratopsids that includes comprehensive sampling of centrosaurines and chasmosaurines 31 ), hadrosauroids 32 , sauropods 33 , and ankylosaurs 34 . Other groups, such as abelisauroid theropods, non-hadrosauroid ornithopods, and non-ceratopsid ceratopsians, could not be analysed because large samples of reasonably complete CampanianMaastrichtian specimens scored for discrete character data are not yet available, almost entirely due to poor fossil sampling [41][42][43] .…”