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THE GALAXY UV LUMINOSITY FUNCTION BEFORE THE EPOCH OF REIONIZATION

  • Authors: Charlotte A. Mason, Michele Trenti, and Tommaso Treu

2015 The Astrophysical Journal 813 21.

  • Provider: AAS Journals

Caption: Figure 9.

Predicted LFs at redshifts z ∼ 2, 5, 10, 16 obtained by calibrating (see Section 2.3) our model with the Finkelstein et al. (2015a) LF at z ∼ 5 (F15, dashed), compared to our reference calibration using the Bouwens et al. (2015a) LF at z ∼ 5 (B15, solid). Shaded regions show the 1σ confidence range, highlighting that within the uncertainty of the calibrations, the two approaches yield consistent results.

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