The X-ray Integral Field Unit (X-IFU) is the high resolution X-ray spectrometer of the ESA
Athena X-ray observatory. Over a field of view of 5'equivalent diameter, it will deliver X-ray …

Extending the earlier measurements reported in Hitomi collaboration (, Nature, 535, 117),
we examine the atmospheric gas motions within the central 100 kpc of the Perseus cluster …

Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster - IOPscience This site
uses cookies. By continuing to use this site you agree to our use of cookies. To find out more …

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 …

Abstract The Hitomi Soft X-ray Spectrometer spectrum of the Perseus cluster, with∼ 5 eV
resolution in the 2–9 keV band, offers an unprecedented benchmark of the atomic modeling …

The metal abundance of the hot plasma that permeates galaxy clusters represents the
accumulation of heavy elements produced by billions of supernovae. Therefore, X-ray …

Much of the baryonic matter in the Universe, including the most active and luminous
sources, are best studied in the X-ray band. Key advances in X-ray optics and detectors …

The resolve instrument onboard the X-Ray Imaging and Spectroscopy Mission (XRISM)
consists of an array of 6× 6 silicon-thermistor microcalorimeters cooled down to 50 mK and a …

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 …

Lynx is an x-ray telescope, one of four large satellite mission concepts currently being
studied by NASA to be a flagship mission. One of Lynx's three instruments is an imaging …