activity
20012021
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 4k across the 78 of their papers we have counts for

collaborators

80 papers

astro-ph.HE2021

The Study of X-Ray Flux Variability of M87

Ryo Imazawa, Yasushi Fukazawa, Hiromitsu Takahashi

We searched for a short-term X-ray variability of the M87 core and jet from archival X-ray data with long exposure data taken by the Suzaku, Chandra, and NuSTAR telescopes. We foun…

astro-ph.HE2021

A study of the accretion mechanisms of the High Mass X-ray Binary IGR J00370+6122

Nagomi Uchida, Hiromitsu Takahashi, Yasushi Fukazawa +1

IGR J00370+6122 is a high-mass X-ray binary, of which the primary is a B1 Ib star, whereas the companion is suggested to be a neutron star by the detection of 346-s pulsation in on…

astro-ph.IM2021★ 23 cited

Detailed Design of the Science Operations for the XRISM mission

Yukikatsu Terada, Matt Holland, Michael Loewenstein +36

XRISM is an X-ray astronomical mission by the JAXA, NASA, ESA and other international participants, that is planned for launch in 2022 (Japanese fiscal year), to quickly restore hi…

astro-ph.IM2021★ 11 cited

Simulations of expected signal and background of gamma-ray sources by large field-of-view detectors aboard CubeSats

Gábor Galgóczi, Jakub Řípa, Riccardo Campana +19

In recent years the number of CubeSats (U-class spacecrafts) launched into space has increased exponentially marking the dawn of the nanosatellite technology. In general these sate…

astro-ph.IM2021★ 2 cited

The simulation framework of the timing-based localization for future all-sky gamma-ray observations with a fleet of Cubesats

Masanori Ohno, Norbert Werner, Andras Pal +22

The timing-based localization, which utilize the triangulation principle with the different arrival time of gamma-ray photons, with a fleet of Cubesats is a unique and powerful sol…

astro-ph.IM2020★ 3 cited

Origin of the in-orbit instrumental background of the Hard X-ray Imager onboard Hitomi

Kouichi Hagino, Hirokazu Odaka, Goro Sato +43

Understanding and reducing the in-orbit instrumental backgrounds are essential to achieving high sensitivity in hard X-ray astronomical observations. The observational data of the…