Fig. 3.

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UV luminosity functions for the Salpeter IMF (red lines) and evolving IMF (blue lines) at z = 6 − 15 including (dark coloured lines) and without (light coloured lines) dust attenuation. Light grey points depict results from observations with the Hubble Space Telescope (Atek et al. 2015, 2018; Bouwens et al. 2021; Castellano et al. 2010; Ishigaki et al. 2018; Livermore et al. 2017; McLeod et al. 2015, 2016; McLure et al. 2013; Oesch et al. 2018; Schenker et al. 2013), while darker grey points show the results from JWST observations (Adams et al. 2024; Bouwens et al. 2023a,b; Donnan et al. 2023a,b, 2024; Finkelstein et al. 2023; McLeod et al. 2024; Harikane et al. 2024; Pérez-González et al. 2023).
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