Fig. 7.

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Predicted 1D and 2D marginalised distributions for the w0–wa and/or γ parameters, for four cosmological model: flat w0waCDM (top left); non-flat w0waCDM (top right); flat w0waγCDM (middle and bottom left); and non-flat w0waγCDM (middle and bottom right). This is for the same scenario as Fig. 6, using the same colour coding (where Euclid-only constraints are here in dashed black). Each plot is accompanied by the corresponding FoM or 1σ uncertainties.
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