Fig. 14.

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Top-heavy PopIII SFRDs (broken lines) from simulations (Maio et al. 2010, 2011a, Pallottini et al. 2014, Xu et al. 2016, Jaacks et al. 2019, Liu & Bromm 2020, Skinner & Wise 2020, Venditti et al. 2023) and semi-analytical models (Visbal et al. 2020, Muñoz et al. 2022, Hegde & Furlanetto 2023, Sarmento & Scannapieco 2025) compared to total SFRD data (solid line) and JWST PopIII determinations (shaded area) taken from Fujimoto et al. (2025).
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