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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 2.

Star formation history, as described by Equation (1) in our model, of a halo of fixed mass 1011 M⊙, if observed at z0 = 2, z0 = 6, or z0 = 10. We label the halo assembly time for the z0 = 2 halo and the mass of the halo progenitor at the start of each constant star formation epoch.

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