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Fig. 2.


BOSS-DR12 anisotropic clustering from Sánchez et al. (2017): the transverse (pink), intermediate (blue) and parallel (black) clustering wedges in two redshift bins, compared with the best-fit cosmological model from our combined multi-probe analysis. The errors, estimated from mock BOSS catalogues (Kitaura et al. 2016), are highly correlated, particularly at large scales (see Fig. A.1).

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