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Fig. D.2.

image

Marginal and 2D posterior distributions for a subset of the cosmological, nuisance, and derived parameters used in our cosmological model. We restrict this figure to only the ‘KV450-DIR δz’ (purple), ‘SOM-Gold Fidicial δz’ (gold), and ‘SOM-Gold noDEEP2 δz’ (green) analyses, as these three analyses encompass the range of posteriors in all of our gold sample analyses (and show similar degeneracies). The joint posterior of AIA and S8 demonstrates that, were a stronger prior on AIA justifiable, agreement between the various gold samples would be even higher.

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