An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models (2015)
Attributed to:
Imperial College Astrophysics & Space Physics Consolidated Grant April 2013 - March 2016
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stv2036
Publication URI: http://dx.doi.org/10.1093/mnras/stv2036
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 2