The fitting results of the observed UV LFs at the redshift range of 4 ≤ z ≤ 9. The selected JWST galaxies are taken from McLure et al. (2013), Finkelstein et al. (2015), Bouwens et al. (2021), Harikane et al. (2022), Adams et al. (2023), Bouwens et al. (2023a), Donnan et al. (2023), Harikane et al. (2023b), Morishita & Stiavelli (2023), and Pérez-González et al. (2023). The solid blue lines depict the best fit to the entire data set. The light blue regions represent the corresponding 90% credible regions. The dashed lines illustrate the best fit of UV LFs but reshaped to the case without dust attenuation. The observational data points are marked in circles with error bars, and the upper limits are shown in lower triangles.