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Fig. 16

image

Monopole and quadrupole of ξ(rp) for the two redshift subsamples of the final VIPERS dataset (solid points), together with the final best-fitting curves obtained using the TNS model, corresponding to the values reported in Table 2. The likelihood computation has used data down to smin = 5 h-1 Mpc, as indicated by the tests. Error bars are 1σ deviations and correspond to the dispersion of the mock measurements. Each of these is also shown as a faint background line.

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