activity
20002025
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 2.9k across the 72 of their papers we have counts for

collaborators

72 papers

astro-ph.HE2025

The unusual spectrum of the X-ray transient source XRISM J174610.8-290021 near the Galactic center

A. Yoshimoto, S. Yamauchi, M. Nobukawa +20

The Galactic center region was observed with the XRISM X-ray observatory during the performance verification phase in 2024 and a point-like X-ray source was detected with the X-ray…

astro-ph.HE2024★ 4 cited

Initial state of the recombining plasma in supernova remnant W 28

Rui Himono, Masayoshi Nobukawa, Shigeo Yamauchi +2

We investigate an SNR W28 with the Suzaku archive data and report the results of spatial resolved analyses. We carry out spectral analysis using a recombining plasma (RP) model wit…

astro-ph.HE2022★ 1 cited

Confirmation of dust scattering echo around MAXI J1421-613 by Swift observation

Kumiko K. Nobukawa, Masayoshi Nobukawa, Shigeo Yamauchi

MAXI J1421-613 is an X-ray burster discovered by Monitor of All-sky X-ray Image (MAXI) on 9 January 2014 and is considered to be a low-mass X-ray binary. A previous study analyzing…

astro-ph.HE2022

Suzaku Observations of Fe K-shell Lines in the Supernova Remnant W51C and Hard X-ray Sources in the Proximity

Aika Shimaguchi, Kumiko K. Nobukawa, Shigeo Yamauchi +2

In this paper, we investigated the Fe K-shell lines in the supernova remnant W51C and hard X-ray sources in the proximity. We measured the intensities of Fe I K and Fe XXV He…

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.HE2021

Spectral and timing properties of the black hole candidate X1755-338 observed in 1989-1995

Shigeo Yamauchi, Sakiho Maeda

We report results of an analysis of the black hole (BH) candidate source X1755-338 in 1989, 1990, and 1991 with Ginga, and in 1995 with ASCA. The spectra were well represented by a…