Ratio of galaxy-event cross-correlation function estimators: ${\mathit{w}}_{DP83}^{\mathrm{stack}}/{\mathit{w}}_{LS93}^{\mathrm{X}-\mathrm{corr}}$ (see Eqs. (2), (3)) as a function of separation in proper kpc. The discrepancy between estimators is smaller than 5% in the range ∼30–∼300 kpc (exact boundaries depending on the samples). For each sample, we fit models on the measurements where the agreement between estimators is better than 5%. For the two highest mass selections, we us the range where the agreement is better than 10%. Differently colored lines represent different samples, identified here by the logarithm of their minimum stellar mass, in solar masses. The color scheme follows that of Fig. 1.