Hiroshi Tsunemi

TL;DR: The XIS is an X-ray imaging spectrometer system, consisting of state-of-the-art charge-coupled devices (CCDs) optimized for Xray detection, camera bodies, and control electronics as mentioned in this paper.

TL;DR: In this paper, the authors summarized the spacecraft, in-orbit performance, operations, and data processing that are related to observations of the Suzaku X-ray observatory, including high-sensitivity wide-band Xray spectroscopy.

TL;DR: X-ray observations of the core of the Perseus cluster reveal a remarkably quiescent atmosphere in which the gas has a line-of-sight velocity dispersion of 164 ± 10 kilometres per second in the region 30–60 kiloparsecs from the central nucleus, infering that a total cluster mass determined from hydrostatic equilibrium in a central region would require little correction for turbulent pressure.

TL;DR: In this article, the sky localization of the first observed compact binary merger is presented, where the authors describe the low-latency analysis of the LIGO data and present a sky localization map.

TL;DR: The newly discovered supernova remnant G266.2-1.2 (RX J0852.0-4622) was observed with ASCA for 120 ks as mentioned in this paper.