Dependence of galaxy clustering on UV luminosity and stellar mass at z ∼ 4

Dependence of galaxy clustering on UV luminosity and stellar mass at z ∼ 4–7

Published:2018-10-01 Issue:4 Volume:481 Page:4885-4894
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Qiu Yisheng¹²,Wyithe J Stuart B¹²,Oesch Pascal A³,Mutch Simon J¹²,Qin Yuxiang¹²^ORCID,Labbé Ivo⁴,Bouwens Rychard J⁵,Stefanon Mauro⁵^ORCID,Illingworth Garth D⁶

Affiliation:

1. School of Physics, University of Melbourne, Parkville, VIC 3010, Australia

2. ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia

3. Department of Astronomy, University of Geneva, Chemin des Maillettes 51, CH-1290 Versoix, Switzerland

4. Centre for Astrophysics & Supercomputing, Swinburne University of Technology, PO Box 218, Hawthorn, VIC 3112, Australia

5. Leiden Observatory, Leiden University, NL-2300 RA Leiden, the Netherlands

6. UCO/Lick Observatory, University of California, Santa Cruz, CA 95064, USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/481/4/4885/25984371/sty2633.pdf

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5. THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROMz= 0-8

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