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)
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