Fig. 4.
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Left panel shows correlation matrix in the case of halo pairwise velocities, while the right panel shows it for the relative velocities between halo pairs in a triplet computed using the 15 000 realisations of the fiducial run of the Quijote suite of simulations. For the right panel, we used all triangular configurations with 20 ≤ r31 ≤ r23 ≤ r12 ≤ 120 h−1 Mpc.
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