(a) The distributions of SN–host angular separation, stellar mass, SFR, and redshift for all hosts from the Pan-STARRS, the Bright Transient Survey (BTS), and the Young Supernova Experiment (YSE), and F. Zou et al. (2022) datasets. Note that the values for Pan-STARRS, BTS, and YSE are inferred by SPLASH while the values from F. Zou et al. (2022) are derived from their SED fits. (b) The distribution of inferred host properties for Type Ia, Ib/c, II, IIn, and SLSNe-I from the OAC with hosts in the Pan-STARRS dataset. We only include hosts with redshifts ≤1 because SPLASH does not classify SNe that are farther away. All histograms are normalized, and the number of hosts for each category (“n”) is included in the legends.