The Galaxy UV Luminosity Function Before the Epoch of Reionization

被引：0

作者：

Mason, Charlotte A. ^{[1
,2
]}

Trenti, Michele ^{[3
]}

Treu, Tommaso ^{[1
,2
]}

机构：

[1] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[2] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA

[3] Univ Melbourne, Sch Phys, Parkville, Vic, Australia

来源：

GALAXIES AT HIGH REDSHIFT AND THEIR EVOLUTION OVER COSMIC TIME | 2016年 / 11卷 / S319期

关键词：

cosmology: theory; galaxies: high-redshift; stars: formation;

D O I：

10.1017/S1743921315009953

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We 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 less than or similar to z less than or similar to 10). We make predictions for reionization and future high-redshift surveys with JWST and WFIRST.

引用

页码：33 / 33

页数：1