Binned UV LFs inferred from our F090W- (left panel), F115W- (middle panel), and F150W-dropout samples (right panel), The orange scatter points indicate the number density of galaxies in fixed M_UV bins. The best-fit Schechter and DPL parameterizations of the UV LF are displayed in, respectively, the solid and dashed colored lines, while the shaded regions indicate the 68% and 95% confidence intervals of the Schechter fits (the confidence intervals of the DPL fits are similar to the Schechter ones, though a little higher at the bright end). For comparison, we also plot number densities based on photometry by S. L. Finkelstein et al. (2015, 2024), R. J. Bouwens et al. (2021), C. T. Donnan et al. (2022, 2024), D. J. McLeod et al. (2024), Y. Harikane et al. (2023), C. J. Willott et al. (2024), N. J. Adams et al. (2024), T. Morishita et al. (2025), L. Whitler et al. (2025), A. Weibel et al. (2026b), and M. Franco et al. (2025, gray symbols), all of which probe survey areas of ∼50 arcmin² or larger. In addition, we plot number densities based on a purely spectroscopic sample by Y. Harikane et al. (2024, 2025) and based on a spectroscopically informed photometric sample by S. Rojas-Ruiz et al. (2025, white scatter points).