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The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at 0 < z < 1.5 (2021)

First Author: Ahad S

Attributed to: Software development support for DiRAC funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stab1036

Publication URI: http://dx.doi.org/10.1093/mnras/stab1036

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2