Little impact of mergers and galaxy morphology on the production and escape of ionizing photons in the early Universe

Open Access

Fig. 3.

Relation between log ξ_ion and M_UV. Each data point corresponds to an individual galaxy in our sample, with different symbols representing the various surveys. We include the curves from Simmonds et al. 2024; Pahl et al. 2025, as well as the relation from Llerena et al. 2025 at z ∼ 6.

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