Constraints on Ω_m, σ₈, α, β, γ, σ_intr, 0, and σ_intr, λ^*, derived in a flat ΛCDM universe by combining the redshift bins z ∈ [0.1,  0.3], z ∈ [0.3,  0.45], and z ∈ [0.45,  0.6] and assuming a minimum intrinsic richness for cluster counts. The shown posteriors were also marginalised over Ω_b, τ, n_s, h, s, q, and δ_b. The blue contours represent the results obtained from the joint analysis of cluster counts and weak lensing masses, while the orange contours show the posteriors on α, β, and γ, derived from the analysis including only the weak lensing masses as in Bellagamba et al. (2019). The confidence ellipses correspond to 68% and 95%, while the bands over the 1D marginalised posteriors represent the 68% of confidence.