Marginalised posterior distributions of the energy contribution due to the cosmological constant. The blue dashed curve indicates the constraints assuming a flat FLRW model. The red curve shows the constraints assuming a ΛLTB model, with radial inhomogeneities in the range r< 3 Gpc, asymptotically embedded into a curved FLRW background. The models were constrained by data from the local Hubble rate, supernovae, the CMB, and kSZ clusters.