Fig. 4.

Download original image
Ratio of galaxy-event cross-correlation function estimators: (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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.