Similar to Fig. 2 but showing the mean relative bias as a function of halo mass for the same set of properties, which are related to the shape (left) and kinematics (right) of the initial clouds. The mean relative bias is simply defined as the ratio between the mean bias of the low- or high-percentile subset and the mean bias of the entire mass bin. Errors were estimated using a bootstrap procedure based on 1000 resampling subsets. The lines connecting data points are simply added to facilitate the readability of the plot.