As in Fig. 3 but for a fixed (FWHM) pseudo-NB width of 600 km s⁻¹ and for different assumed clustering strengths for undetected sources, depending on their Lyα luminosity. The red and blue enhancement factors assume that undetected LAEs cluster similarly to MUSE-Wide and MXDF LAEs, respectively. The orange, gray, and green factors assume an extrapolated HOD 2pcf for LAEs with log(L_Lyα/[erg s⁻¹]) ≈ 40.0, log(L_Lyα/[erg s⁻¹]) ≈ 38.5, and log(L_Lyα/[erg s⁻¹]) ≈ 37.0, respectively. In all cases, detected LAEs cluster similarly to what is seen for the MUSE-Wide sample.