Image Details
Caption: Figure 3.
The theoretical predictions of the ultraviolet luminosity functions ﹩{\mathrm{log}}_{10}{\rm{\Phi }}﹩ at high redshifts (z ∼ 10, 11, and 12) in four EDE models (upper panels), along with their residuals Δ log10Φ relative to the best-fit ΛCDM model (lower panels). The data points with error bars represent the high-redshift observations from JWST.
© 2026. The Author(s). Published by the American Astronomical Society.