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Fig. 3.


Cross-correlation data computed on Herschel SMGs (as background sample) and GAMA galaxies (as lenses sample). The grey points are exactly the results obtained in González-Nuevo et al. (2017). The red data set (obtained using the same binning as in González-Nuevo et al. 2017) and the blue data set (obtained using same the binning, but half-size bin shifted with respect to González-Nuevo et al. 2017) are the cross-correlation results computed for this work, exploiting a larger area. The solid lines represent the best fit with flat priors to the astrophysical and cosmological parameters using the default binning (red) and the shifted binning (blue). The green line is the best fit to the red case, but adopting Ωm = 0.3.

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