Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S319(11), p. 33-33, 2015

DOI: 10.1017/s1743921315009953

American Astronomical Society, Astrophysical Journal, 1(813), p. 21, 2015

DOI: 10.1088/0004-637x/813/1/21

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The Galaxy UV Luminosity Function Before the Epoch of Reionization

Journal article published in 2015 by Charlotte A. Mason ORCID, Michele Trenti ORCID, Tommaso Treu ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe present a model for the evolution of the galaxy ultraviolet (UV) luminosity function (LF) where star formation is linked to the assembly of dark matter halos under the assumption of a mass dependent, but redshift independent, efficiency. With a calibration at a single redshift, and no further degrees of freedom, our model captures the evolution of the UV LF over all available observations (0≲ z ≲ 10). We make predictions for reionization and future high-redshift surveys with JWST and WFIRST.

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