HI properties and galaxy properties for the (e)LARS sample and optically-selected galaxies from SDSS-ALFALFA (Durbala et al. 2020). In all panels, we split the (e)LARS sample between objects considered Lyα emitters (EW_Lyα ≥ 20 Å, in black) and weak and non-emitters (EW_Lyα < 20 Å, in gray). The SDSS/ALFALFA galaxies are shown in blue. Squares indicate the median in stellar mass or HI mass bins, blue squares show the median for the SDSS/ALFALFA galaxies, black squares the median for the (e)LARS Lyα-emitters, and gray squares the median for the weak and non Lyα-emitters. The error bars associated with the median points show the standard deviation within a given mass bin. In the top-left panel, the solid black line shows the SFMS at z = 0 (Speagle et al. 2014).