Left: Revised Fig. 2 from Daddi et al. (2022b) showing the distribution of LANs in this work (blue points) and previous KCWI observations (red points) across the plane of L_Lyα/BAR-M_stream/M_h. The green line is the best fit in Daddi et al. (2022b) revised using the modified M_stream in Daddi et al. (2022a). Right: Revised Fig. 3 from Sillassen et al. (2024) showing how massive galaxy groups in this work (blue points), Coogan et al. (2023) (orange points), previous KCWI observations (Daddi et al. 2022b, black points), and the NICE survey (Zhou et al. 2024 in red points and Sillassen et al. 2024 in green points) are distributed across the SFR_IR/BAR-M_stream/M_h plane. The green line is the original best fit in Sillassen et al. (2024). In both panels, black lines show the revised best fits of Eq. (4) in Daddi et al. (2022b) with α_Lyα = 0.87 ± 0.19 (left) and of Eq. (5) in Sillassen et al. (2024) with α_SFR = 0.70 ± 0.15 (right) after adding RO-1001-Sat and RO-0959-Sat into the fits.