THE GALAXY UV LUMINOSITY FUNCTION BEFORE THE EPOCH OF REIONIZATION
Charlotte A Mason, Michele Trenti, Tommaso Treu
The Astrophysical Journal: an international review of astronomy and astronomical physics | IOP PUBLISHING LTD | Published : 2015
We present a model for the evolution of the galaxy ultraviolet (UV) luminosity function (LF) across cosmic time where star formation is linked to the assembly of dark matter halos under the assumption of a mass-dependent, but redshift-independent, efficiency. We introduce a new self-consistent treatment of the halo star formation history, which allows us to make predictions at z > 10 (lookback time ≲500 Myr), when growth is rapid. With a calibration at a single redshift to set the stellar-to-halo mass ratio, and no further degrees of freedom, our model captures the evolution of the UV LF over all available observations (0 ≲ z ≲ 10). The significant drop in luminosity density of currently det..View full abstract
Awarded by HST BoRG
Awarded by HST GLASS grant
This work was supported by the HST BoRG grants GO-12572, 12905, and 13767, and the HST GLASS grant GO-13459. T.T. acknowledges support by the Packard Foundation through a Packard Fellowship.