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Fig. 2.

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CCF data computed on Herschel SMGs (as background sample) and GAMA galaxies (as lenses sample) in the mini-Tiles data sets (red points) for the different redshift bins (from left to right, top to bottom): 0.1–0.2 (Bin1), 0.2–0.3 (Bin2), 0.3–0.5 (Bin3), and 0.5–0.8 (Bin4). The empty circles are the data discarded from the MCMC analysis, as explained in the text. The best fits performed in this work are also shown: the runs allowing for astrophysical parameters only (solid line) and for astrophysical and cosmological parameters: σ8, ΩM, and h (dotted line); σ8, ΩM, h, and ω0 (dashed line); and σ8, ΩM, h, ω0, and ωa (dash-dotted line). In the left panel the peaks of the marginalised 1D posterior distributions are used, and in the right panel the mean is used.

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