Comparison of galaxy properties between z ∼ 0.3 LyC emitters from the LzLCS+ Flury et al. 2022b and high-redshift sources, shown as a density plot. Panels show log M_⋆ vs. β slope (top), M_UV vs. β (middle), and E(B-V) vs. β (bottom). Of the 88 LyC emitters, 51 galaxies are identified as analogs to high-redshift sources, falling within the 99% confidence interval in all panels. Known LyC leakers at z ∼ 3 are also included from the literature: Ion1 Vanzella et al. 2012, Ion2 Vanzella et al. 2015, 2016; de Barros et al. 2016, Ion3 Vanzella et al. 2018, J1316+2614 Marques-Chaves et al. 2022, CDFS-6664 Yuan et al. 2021, LACES Fletcher et al. 2019, and samples from Kerutt et al. 2024 and Jung et al. 2024b. All the known leakers are color-coded by their log₁₀(f_esc).