activity
20162024
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 777 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM20246 cited

High-speed Readout System of X-ray CMOS Image Sensor for Time Domain Astronomy

Naoki Ogino, Makoto Arimoto, Tatsuya Sawano +6

We developed an FPGA-based high-speed readout system for a complementary metal-oxide-semiconductor (CMOS) image sensor to observe soft X-ray transients in future satellite missions…

astro-ph.HE20238 cited

A broadband X-ray imaging spectroscopy in the 2030s: the FORCE mission

Koji Mori, Takeshi G. Tsuru, Kazuhiro Nakazawa +49

In this multi-messenger astronomy era, all the observational probes are improving their sensitivities and overall performance. The Focusing on Relativistic universe and Cosmic Evol…

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.HE201623 cited

X-ray and Rotational Luminosity Correlation and Magnetic Heating of the Radio Pulsars

S. Shibata, E. Watanabe, Y. Yatsu +2

Previous works have suggested a correlation between the X-ray luminosity Lx and the rotational luminosity Lrot of the radio pulsars.However, none of the obtained regression lines a…

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…