Notes. The galaxy properties are summarised by: the mean redshift, ⟨z⟩; the number of galaxies in the density (shape) sample, N_D (N_S); the mean luminosity in terms of a pivot luminosity L₀ = 4.6 × 10¹⁰ h⁻² L_⊙; the bias, b_g. To compute the ratio ⟨L⟩/L₀, we only consider the galaxies in the corresponding shape sample. For our L-cuts sub-samples, we also provide the range in luminosity they probe, [L_min, L_max], in units of 10¹⁰ h⁻² L_⊙. Similarly, we provide in brackets the cut adopted to split our sample in two redshift bins. When cross-correlating different samples, N_D refers to the density sample used in the correlation and the bias is the best-fit bias of the density tracer as obtained for that given measurement. All measurements are performed assuming Π_max = 120 h⁻¹ Mpc. Since the best-fit parameters and the medians of the marginal posterior distributions are in agreement, we quote the marginal values, while the χ² refers to the maximum likelihood. In all cases, the degrees of freedom are 5; the p-values are all above 0.03, with the majority of them being in the range 0.3–0.7.