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Fig. A.2.

Fig. A.2. Refer to the following caption and surrounding text.

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Joint marginal error contours at 1 σ and 2 σ on a subset of the cosmological parameters for a flat f(R) model with |fR0| = 5 × 10−6 (HS6). In solid orange the combination of GCsp and WL and in red contour lines the 3×2 pt combination of photometric probes. It can be seen that it is the spectroscopic probes driving the constraints on Ωb, 0 and h, which in combination with WL helps break degeneracies.

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