Robert Petre

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 paper, X-ray observations of the remnant of supernova 1006, made by the ASCA satellite, indicate that emission from the edges of the supernova remnant shell is dominated by radiation from electrons accelerated to energies of ~ 100 TeV within the shock front.

TL;DR: The Advanced Telescope for High Energy Astrophysics (Athena+) mission as discussed by the authors provides the necessary performance (e.g., angular resolution, spectral resolution, survey grasp) to address these questions and revolutionize our understanding of the Hot and Energetic Universe.

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 paper, the authors observed the C/Hyakutake 1996 B2 at extreme ultraviolet and x-ray wavelengths with the Rœntgen Xray Satellite and Rossi X-ray Timing Explorer.