Yuzuru Tawara

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: In this article, the design parameters, production process, and in-flight performance of the X-ray telescopes (XRTs) onboard Suzaku were presented. And the optical axes were found to be distributed within a radius of 1. 0 8 −2.

TL;DR: In this paper, the authors reported the discovery of intense iron-line emission at 6.7 keV from the Galactic Centre, detected by the Ginga satellite, with characteristics consistent with its production by a shock-heated plasma.

TL;DR: The ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science (ISAS) as discussed by the authors.

TL;DR: In this article, high-resolution mm-wave observations of the interstellar CO molecule have revealed molecular gas at 1kpc distance interacting with the TeV γ-ray SNR G 347.5, and that a molecular cloud of ∼ 200 solar masses is clearly associated with the supernova peak, providing strong evidence for proton acceleration.