Clustering dependencies on object properties. Top left: clustering variation in two different redshift subsamples. The blue dots show the clustering in the lower redshift bin while the red points show the higher redshift subsample. The dotted curves represent the best HOD fits. Top right: same details but for two different Lyα luminosity subsamples. Bottom left: same details but for EW_Lyα. Bottom right: same details but for UV absolute magnitude. The black line represents the K expectation value for an unclustered sample of galaxies and the 1σ error bars are determined from the bootstrapping approach explained in Sect. 3.1.3.