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Fig. 5

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Bayesian MCMC analysis of the fiducial survey estimating the matter band power (left; relative to the fiducial power spectrum) and the galaxy biasing parameters (middle: bias factor; right: correlation factor). The shadowed area in the background highlights a 68% credibility region about the marginalised posterior mean for the lowest redshift bin , whereas data points delineate the 68% credibility regions about the mean at higher redshifts. The highest, most poorly constrained redshift bin is not included here. The results are subject to some numerical noise caused by the adopted MCMC technique.

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