Open Access

Fig. 10.


Same as Fig. 6, but employing a different prior power spectrum (Ωm = 0.40, w0 = −0.85), for ∼3000 MCMC realisations. By recovering the fiducial cosmological parameters employed in the mock generation, this test case explicitly highlights the robustness of our approach to the shape of the prior power spectrum adopted. The corresponding uncertainties are slightly larger than for the original run by around 15%.

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