Fig. 7.
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Location of our two LyC candidate leakers (stars) in the β vs. stellar mass (left) and β vs. MUV (right) diagrams, compared to known leakers at z ∼ 0.3 (Flury et al. 2022b) and z > 2 (Vanzella et al. 2016, 2018, 2020; Marques-Chaves et al. 2022; Kerutt et al. 2024; Jung et al. 2024). The sources are color-coded based on their log10fesc values. A typical error bar is shown in the bottom right corner of each figure.
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