Secondary halo bias (measured at z = 0) produced by a set of properties related to the shape (left) and kinematics (right) of the collapsing regions at z = 12 from which z = 0 halos in specific mass bins originate. These results are compared with the assembly bias signal, represented here by the concentration, c_vir, secondary dependence. The mean biases in equal-size percentile subsets encompassing halos with the 20% lowest and highest values of the corresponding property in each mass bin are shown as a function of halo mass, along with the mean bias of the entire population in that mass bin. Errors were estimated using a bootstrap technique based on 1000 resampling subsets. The lines connecting data have been added only for the sake of a better visualization of the differences between subsets.