Image Details

Choose export citation format:

z ∼ 2–9 Galaxies Magnified by the Hubble Frontier Field Clusters. II. Luminosity Functions and Constraints on a Faint-end Turnover

  • Authors: R. J. Bouwens, G. Illingworth, R. S. Ellis, P. Oesch, M. Stefanon

R. J. Bouwens et al 2022 The Astrophysical Journal 940 .

  • Provider: AAS Journals

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.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse