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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 13.

Similar to Figure 12, but for the Delphi model (Dayal et al. 2014, 2022), FirstLight (Ceverino et al. 2017), ASTRAEUS-EarlyHeating (Hutter et al. 2021), ASTRAEUS-JeanMass (Hutter et al. 2021), ENZO (O’Shea et al. 2015), THESAN project (Kannan et al. 2022), and Yue et al. (2016; Y16). Also shown with the red line is the abundance matching constraints on the LF at z ∼ 7 from the Boylan-Kolchin et al. (2015) analysis.

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