Bolometric luminosity (L_bol), Eddington ratio (λ_Edd), star formation rate (SFR), and stellar mass (M_*) as a function of the relative extent of H I gas including low-density gas (D_HI, ext) to stellar disk (D₂₅). L_bol and λ_Edd are adopted from BASS DR2 (Koss et al. 2022a). Each galaxy is colored by the hard X-ray luminosity adopted from Ricci et al. (2017). On each panel, the Spearman rank correlation (S) and the Pearson correlation (P) coefficient, and a p-value between each axis are shown at the bottom. There is a marginal, linear correlation between L_bol and the H I extent in the sense that galaxies with a relatively larger H I disk compared to the stellar disk are more luminous. This also applies to the Eddington ratio, whereas the relative size of H I does not seem to be related to SFR. M_* appears to show a marginal negative correlation with D_HI, ext/D₂₅, which is naturally expected, as D_HI, ext is normalized by D₂₅.