activity
20142019
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 867 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE201937 cited

Observations of a Pre-Merger Shock in Colliding Clusters of Galaxies

Liyi Gu, Hiroki Akamatsu, Timothy W. Shimwell +10

Clusters of galaxies are the largest known gravitationally-bound structures in the Universe. When clusters collide, they create merger shocks on cosmological scales, which transfor…

astro-ph.HE201944 cited

X-ray spectra of the Fe-L complex

Liyi Gu, A. J. J. Raassen, Junjie Mao +7

The Hitomi results on the Perseus cluster lead to improvements in our knowledge of atomic physics which are crucial for the precise diagnostic of hot astrophysical plasma observed…

astro-ph.HE2017116 cited

Solar abundance ratios of the iron-peak elements in the Perseus Cluster

Hitomi Collaboration

The metal abundance of the hot plasma that permeates galaxy clusters represents the accumulation of heavy elements produced by billions of supernovae. Therefore, X-ray spectroscopy…

astro-ph.HE201619 cited

Suzaku and XMM-Newton Observations of the North Polar Spur: Charge Exchange or ISM Absorption?

Liyi Gu, Junjie Mao, Elisa Costantini +1

By revisiting the Suzaku and XMM-Newton data of the North Polar Spur, we discovered that the spectra are inconsistent with the traditional model consisting of pure thermal emission…

astro-ph.GA2016500 cited

The Quiescent Intracluster Medium in the Core of the Perseus Cluster

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +213

Clusters of galaxies are the most massive gravitationally-bound objects in the Universe and are still forming. They are thus important probes of cosmological parameters and a host…

astro-ph.HE2016124 cited

Hitomi constraints on the 3.5 keV line in the Perseus galaxy cluster

Hitomi Collaboration, Felix A. Aharonian, Hiroki Akamatsu +215

High-resolution X-ray spectroscopy with Hitomi was expected to resolve the origin of the faint unidentified E=3.5 keV emission line reported in several low-resolution studies of va…