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The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin (2020)

First Author: Bhargava S

Attributed to: Lancaster University Astrophysics funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa1829

Publication URI: http://dx.doi.org/10.1093/mnras/staa1829

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 1