Proper motion distributions for the different clusters. The field stars within FOV_20pc that have absolute proper motions ≤75 mas yr⁻¹ and the member stars are indicated in black and yellow, respectively. The top-left sub-panels focus on the proper motions of the members; the blue and red circles correspond to those identified within FOV_20pc and FOV_2pc, respectively. Typical (mean) uncertainties in proper motions are ∼0.04 mas yr⁻¹, roughly comparable to the size of such circles for most cases.