activity
20002025
most citedHigh Resolution X-ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies

554 citations · 1.6k across the 17 of their papers we have counts for

collaborators

18 papers

astro-ph.IM2025

In orbit operation of Resolve Filter Wheel and MXS

Russell F. Shipman, Shunji Kitamoto, Rob Wolfs +17

The Resolve soft X-ray spectrometer is the high spectral resolution microcalorimeter spectrometer for the XRISM mission. In the beam of Resolve there is a filter wheel containing \…

astro-ph.IM2020★ 13 cited

An online data analysis system of INTEGRAL telescope

A. Neronov, V. Savchenko, A. Tramacere +3

During more than 17 years of operation in space INTEGRAL telescope has accumulated large data set that contains records of hard X-ray and soft gamma-ray astronomical sources. These…

astro-ph.HE2018★ 267 cited

An embedded X-ray source shines through the aspherical AT2018cow: revealing the inner workings of the most luminous fast-evolving optical transients

Raffaella Margutti, B. D. Metzger, R. Chornock +41

We present the first extensive radio to gamma-ray observations of a fast-rising blue optical transient (FBOT), AT2018cow, over its first ~100 days. AT2018cow rose over a few days t…

astro-ph.HE2017★ 43 cited

Temperature Structure in the Perseus Cluster Core Observed with Hitomi

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +192

The present paper investigates the temperature structure of the X-ray emitting plasma in the core of the Perseus cluster using the 1.8--20.0 keV data obtained with the Soft X-ray S…

astro-ph.HE2014★ 3 cited

ASTRO-H White Paper - Accreting Pulsars, Magnetars, and Related Sources

S. Kitamoto, T. Enoto, S. Safi-Harb +18

As the endpoints of massive star evolution, neutron stars are enigmatic celestial objects characterized by extremely dense and exotic nuclear matter, magnetospheres with positrons…

astro-ph.HE2014★ 2 cited

ASTRO-H White Paper - Low-mass X-ray Binaries

C. Done, M. Tsujimoto, E. Cackett +20

There is still 10-20% uncertainty on the neutron star (NS) mass-radius relation. These uncertainties could be reduced by an order of magnitude through an unambiguous measure of M/R…