Fig. 4.
Galaxy clustering (top panel) and position-intrinsic shear correlations (bottom panel) measured in the full KiDS+GAMA and SDSS Main datasets. Solid lines illustrate the best-fit NLA model, and dot-dashed lines the LA. The vertical dashed line indicates rp = 6 h−1 Mpc, below which scales are excluded from fitting (Sect. 3.3).
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