Performance of ASTRO-H Hard X-Ray Telescope (HXT)

Abstract: The Japanese X-ray Astronomy Satellite, Hitomi (ASTRO-H) carries hard X-ray imaging system, covering the energy…

First Peek of ASTRO-H Soft X-Ray Telescope (SXT) In-Orbit Performance

Abstract: ASTRO-H (Hitomi) is a Japanese X-ray astrophysics satellite just launched in February, 2016, from Tanegashima,…

Electromagnetic Cyclotron Waves in the Solar Wind: Wind Observation and Wave Dispersion Analysis

Abstract: Wind observed long-lasting electromagnetic cyclotron waves near the proton cyclotron frequency on 11 March 2005,…

The Merging Galaxy Cluster A520 – A Broken-Up Cool Core, A Dark Subcluster, and an X-Ray Channel

Abstract: We present results from a deep Chandra X-ray observation of a merging galaxy cluster A520.…

Radial Profile of the 3.5 kev Line Out to R200 in the Perseus Cluster

Abstract: The recent discovery of the unidentified emission line at 3.5 keV in galaxies and clusters…

Spiral Structure and Differential Dust Size Distribution in the LkH(alpha) 330 Disk

Abstract: Dust trapping accelerates the coagulation of dust particles, and, thus, it represents an initial step…

A Comprehensive Radial Velocity Error Budget for Next Generation Doppler Spectrometers

Abstract: We describe a detailed radial velocity error budget for the NASA-NSF Extreme Precision Doppler Spectrometer…

Space Telescope and Optical Reverberation Mapping Project. VI. Reverberating Disk Models for NGS 5548

Abstract: We conduct a multi-wavelength continuum variability study of the Seyfert 1 galaxy NGC 5548 to…

Imaging Analysis of the Hard X-Ray Telescope ProtoEXIST2 and New Techniques for High-Resolution Coded-Aperture Telescopes

Abstract: Wide-field (greater than or approximately equal to 100 degrees squared) hard X-ray coded-aperture telescopes with…

The Weak Fe Fluorescence Line and Long-Term X-Ray Evolution of the Compton-Thick Active Galactic Nucleus in NGC7674

Abstract: We present NuSTAR X-ray observations of the active galactic nucleus (AGN) in NGC7674.The source shows…