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Fig. B.1.


Impact of the ns prior: Comparing marginalised posterior distributions for the BOSS galaxy clustering analysis for our fiducial analysis (blue) with the constraints when adopting an uninformative prior on ns (orange). Opening the parameter space to arguably unphysical values of ns favours higher values and weaker constraints on Ωm. Constraints on S8 are, however, fairly insensitive to the choice of ns prior.

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