Lynx, one of the four strategic mission concepts under study for the 2020 Astrophysics
Decadal Survey, provides leaps in capability over previous and planned x-ray missions and …

Both heliophysics and planetary physics seek to understand the complex nature of the solar
wind's interaction with solar system obstacles like Earth's magnetosphere, the ionospheres …

Hard X-ray (≥ 10 keV) observations of active galactic nuclei (AGNs) can shed light on some
of the most obscured episodes of accretion onto supermassive black holes. The 70-month …

High-sensitivity wide-band X-ray spectroscopy is the key feature of the Suzaku X-ray
observatory, launched on 2005 July 10. This paper summarizes the spacecraft, in-orbit …

This paper presents development of an X-ray pixel detector with a multi-port charge-coupled
device (MPCCD) for X-ray Free-Electron laser experiments. The fabrication process of the …

High-frequency gravitational waves (HFGWs) carry a wealth of information on the early
Universe with a tiny comoving horizon and astronomical objects of small scale but with …

Abstract The Hard X-ray Detector (HXD) on board Suzaku covers a wide energy range from
10 keV to 600 keV by the combination of silicon PIN diodes and GSO scintillators. The HXD …

We present a new X-ray spectroscopic study of 22 luminous (2× 10 45≲ L bol/erg s− 1≲ 2×
10 46) active galactic nuclei (AGNs) at intermediate redshifts (0.1≲ z≲ 0.4), as part of the …

We present the design parameters, production process, and in-flight performance of the X-
ray telescope (XRT) onboard Suzaku. The imaging capability is significantly improved over …

We detect a line at 3.539±0.011 keV in the deep exposure data set of the Galactic center
region, observed with the x-ray multi-mirror mission Newton. The dark matter interpretation …