Fig. 8.

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Escape fraction fesc against O32 ratio for a number of different LyC leakers. These include the LzLCS (z = 0.2–0.4, blue points; Saldana-Lopez et al. 2022; Flury et al. 2022) and other low-redshift massive starbursts from Roy et al. (2024). We also plot detections and lower limits (pink points) from Nakajima et al. (2020) and the high fesc average from Naidu et al. (2022a), all of which are z = 2–3. As orange points, we plot values from Saxena et al. (2024, in some cases O32 lower limits) with fesc calculated from the βUV slope via the Chisholm et al. (2022) method. We report the value of the SED fit fesc as the red square and that of the Chisholm et al. (2022) fesc as the turquoise diamond. We observed that JADES-GS8-RL-1 is clearly in a totally different region of the diagram compared to all the other galaxies due to the unusual combination of high fesc and extremely low O32.
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