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An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models (2015)

First Author: Mead A

Attributed to: Astronomy and Astrophysics at Edinburgh 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