Left: rest-frame EW distribution for SFGs with Lyα in emission (positive EWs) and Lyα in absorption (negative EWs). The vertical dashed line indicates EW = 20 Å, the adopted lower limit in Lyα EW for LAEs (or strong Lyα emitters). The solid curve is the KDE of the distribution. Middle: distribution of Lyα luminosities for the SFG_L (black) and the LAE (red) samples. The KDE of the distribution is shown by a solid curve. Right: fraction of LAEs as a function of redshift for our sample. Approximately 10% of SFGs at these redshifts are strong Lyα emitters, consistent with previous Lyα studies (e.g., Reddy et al. 2008; Cassata et al. 2015) at similar redshifts.