Fig. 8.
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Evolution of the cosmic UV density for galaxies with MUV < −17. FirstLight values are above the models with redshift-independent efficiency by Harikane et al. (2022) and Tacchella et al. (2018), as well as other pre-JWST observations at z ≥ 10 (Oesch et al. 2018). JWST values (Harikane et al. 2023; McLeod et al. 2024; Chemerynska et al. 2024; Donnan et al. 2024) are consistent with FirstLight within the estimated uncertainties.
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