Fig. F.1.
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Galaxy-galaxy covariance contraction for the RC25 model with the same parameterization than 6 (and σg = 3.0 h−1·Mpc) while varying the reference position r1 in the parallel r1,∥ (left) and perpendicular r1,⊥ (right) direction. Those contractions are expressed in one-dimension as a function of perpendicular separation r⊥ when r∥ = 0 h−1·Mpc.
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