The evolution of K* and the halo occupation distribution since z= 1.5: observations versus simulations The evolution of K* and the HOD since z= 1.5 (2012)

First Author: Capozzi D
Attributed to:  Astrophysics Research at Liverpool John Moores University funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2011.19895.x

Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2011.19895.x

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 4