Fig. 6.

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For the w0waCDM model, comparison of each of the Fisher marginalised (light grey) and unmarginalised (dark grey) errors on each cosmological and nuisance parameter for: photometric optimistic probe (top left); photometric pessimistic probe (top right); spectroscopic optimistic probe (bottom left); and spectroscopic pessimistic probe (bottom right). For the spectroscopic probe the labels lbsi are short for the parameters ln(b σ8)i.
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