Clusters of galaxies are the most massive gravitationally bound objects in the Universe and
are still forming. They are thus important probes of cosmological parameters and many …

The most massive baryonic component of galaxy clusters is the 'intracluster medium'(ICM), a
diffuse, hot, weakly magnetized plasma that is most easily observed in the X-ray band …

The X-ray Integral Field Unit (X-IFU) on board the Advanced Telescope for High-ENergy
Astrophysics (Athena) will provide spatially resolved high-resolution X-ray spectroscopy …

Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster - IOPscience This site
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The Hitomi (ASTRO-H) mission is the sixth Japanese x-ray astronomy satellite developed by
a large international collaboration, including Japan, USA, Canada, and Europe. The mission …

We present the overall design and performance of the Astro-H (Hitomi) Soft X-Ray
Spectrometer (SXS). The instrument uses a 36-pixel array of x-ray microcalorimeters at the …

The Hitomi (ASTRO-H) mission is the sixth Japanese X-ray astronomy satellite developed by
a large international collaboration, including Japan, USA, Canada, and Europe. The mission …

We present an analysis of ionized X-ray disk winds found in the Fe K band of four stellar-
mass black holes observed with Chandra, including 4U 1630− 47, GRO J1655− 40, H …

X-ray surface brightness fluctuations in the core of the Perseus Cluster are analysed, using
deep observations with the Chandra observatory. The amplitude of gas density fluctuations …

Abstract Cerium-doped Gd 3 (Ga, Al) 5 O 12 (GAGG: Ce) is a promising novel scintillator for
gamma-ray detectors. While GAGG: Ce has already been implemented in various …