Notes. Expressed in mas yr⁻¹. Both systemic motions are referred to the LMC photometric centre (α_c, δ_c) = (81.28^∘, −69.78^∘), by van der Marel (2001). A kinematic model fit is used in Gaia Collaboration (2021b) to derive the systemic motion (see their Table 5, Main model). In this work, the systemic motion is re-derived by computing the median velocity within a 0.5^∘ with respect to the LMC centre, where uncertainties are derived as MAD/$\sqrt{N}$.