Detected (or upper limit) f_esc values versus the predicted f_esc values ftom Cox models, calibrated using the full LzLCS+ sample and the subsample of galaxies resembling reionization-era sources. Left panel: Predictions using the ELG-EW model. Right panel: Predictions using the ELG-O32 model. The Cox models from Jaskot et al. 2024b are shown in blue, while predictions calibrated on the subsample are in red. Predictions applied to known LyC leakers at z ∼ 3 are also shown in red Vanzella et al. 2015, 2016; de Barros et al. 2016; Marques-Chaves et al. 2022; Fletcher et al. 2019; Kerutt et al. 2024. Upper limits are indicated with downward-pointing arrows.