Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations (2019)

First Author: Okabe Nobuhiro
Attributed to:  Research in planetary formation, astrophysics, and cosmology at Bristol funded by STFC

Abstract

No abstract provided

Bibliographic Information

Type: Journal Article/Review

Parent Publication: arXiv e-prints