Image Details
Caption: Figure 5.
The 68% likelihood contours we derive on the shape of the faint end of the UV LFs at z ∼ 2, z ∼ 3, z ∼ 4, z ∼ 5, z ∼ 6, z ∼ 7, z ∼ 8, and z ∼ 9 based on our lensed HFF samples and the presented constraints on the LF from blank-field studies. The solid circles show our LF constraints from the Bouwens et al. (2021a) blank-field analysis. The z ∼ 10 LF results shown here are from Oesch et al. (2018a) and rely on both blank-field and lensing-field results.
© 2022. The Author(s). Published by the American Astronomical Society.