The XMM Cluster Survey: new evidence for the 3.5 keV feature in clusters is inconsistent with a dark matter origin (2020)
Attributed to:
University of Sussex Astronomy Consolidated Grant 2017-2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2006.13955
Publication URI: https://arxiv.org/abs/2006.13955
Type: Other