Fig. 6.

Foreseen constraints (1σ contours) for a set of five ΛCDM parameters, plus three galaxy bias parameters (out of a total of 20) for a DESI-like survey. We assume 20 tomographic Gaussian bins of size σz = 0.01. The blue lines are the constraints for angular galaxy clustering alone Dg, the orange lines are for the ARF alone Dz, and the green line is a joint analysis of both fields Dg, z. The figures above the 1-D PDFs give the marginalised 1σ uncertainty of the parameter for each data vector. We show here only three galaxy bias parameters, even if we marginalised upon the 20 bias parameters.
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