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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 1.

Efficiency of star formation, the ratio of stellar mass formed during the halo assembly time to halo mass, see Equation (2), derived at the calibration redshift z ∼ 5, as described in Section 2.3. The shaded region shows 1σ confidence range.

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