UV luminosity function at different redshifts in the cold (black), fuzzy (green), and warm (orange) DM models and in the model with enhanced matter power (red). The best fit is shown for CDM and WDM cases, while for FDM the mass corresponds to the 95% lower bound. The dashed and dot-dashed curves show the CDM UV luminosity function without the suppression of the feedback effects and without the change in the UV conversion factor κ_UV. The points with errorbars show the HST measurements from Bouwens et al. (2021) (cyan) and Harikane et al. (2022) (pink) and the JWST measurements from Donnan et al. (2024) (blue), Pérez-González et al. (2025) (brown), and Castellano et al. (2025) (grey).