“…1(b)], which precisely cover the Γ-M lines. The streaks are, in fact, quasi-2D objects (independent of Q ⊥ ) in reciprocal space, which correspond to quasi-1D correlations in real space, and they can be viewed as a 2D counterpart of rod-like diffuse scattering in Yb 2 Ti 2 O 7 [64,65], which has been attributed to coexisting FM and AFM correlations [66,67]. Below T N , the body of the star is depleted, including the FM-like diffuse scattering near Γ [Fig.…”