Search Publications
X-Ray Imaging Spectrometer (XIS) on Board Suzaku
Hamaguchi, Kenji; Dotani, Tadayasu; Miller, Eric D. +43 more
The XIS is an X-ray Imaging Spectrometer system, consisting of state-of-the-art charge-coupled devices (CCDs) optimized for X-ray detection, camera bodies, and control electronics. Four sets of XIS sensors are placed at the focal planes of the grazing-incidence, nested thin-foil mirrors (XRT: X-Ray Telescope) onboard the Suzaku satellite. Three of…
The X-Ray Observatory Suzaku
Hamaguchi, Kenji; White, Nicholas E.; Isobe, Naoki +140 more
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 performance, operations, and data processing that are related to observations. The scientific instruments, the high-throughput X-ray telescopes, X-ray CCD cameras, non-imaging ha…
Hard X-Ray Detector (HXD) on Board Suzaku
Isobe, Naoki; Yamaoka, Kazutaka; Fukazawa, Yasushi +66 more
The Hard X-ray Detector (HXD) on board Suzaku covers a wide energy range from 10keV to 600keV by the combination of silicon PIN diodes and GSO scintillators. The HXD is designed to achieve an extremely low in-orbit background based on a combination of new techniques, including the concept of a well-type active shield counter. With an effective are…
The X-Ray Telescope onboard Suzaku
Maeda, Yoshitomo; Ishida, Manabu; Kunieda, Hideyo +31 more
Monte Carlo Simulator and Ancillary Response Generator of Suzaku XRT/XIS System for Spatially Extended Source Analysis
Hamaguchi, Kenji; Miller, Eric D.; Maeda, Yoshitomo +31 more
We have developed a framework for the Monte Carlo simulations of X-Ray Telescope (XRT) and X-ray Imaging Spectrometer (XIS) on board Suzaku, mainly for the scientific analysis of spatially and spectroscopically complex celestial sources. A photon-by-photon instrumental simulator is built on the ANL platform, which has been successfully used in ASC…
In-Orbit Performance of the Hard X-Ray Detector on Board Suzaku
Isobe, Naoki; Enoto, Teruaki; Yamaoka, Kazutaka +55 more
The in-orbit performance and calibration of the Hard X-ray Detector (HXD) on board the X-ray astronomy satellite Suzaku are described. Its basic performances, including a wide energy bandpass of 10-600keV, energy resolutions of ∼4keV (FWHM) at 40keV and ∼11% at 511keV, and a high background rejection efficiency, have been confirmed by extensive in…
Suzaku Observations of the Hard X-Ray Variability of MCG -6-30-15: the Effects of Strong Gravity around a Kerr Black Hole
Fabian, Andrew C.; Kunieda, Hideyo; Haba, Yoshito +21 more
Suzaku has, for the first time, enabled the hard X-ray variability of the Seyfert 1 galaxy MCG -6-30-15 to be measured. The variability in the 14-45keV band, which is dominated by a strong reflection hump, is quenched relative to that at a few keV. This directly demonstrates that the whole reflection spectrum is much less variable than the power-l…
Evidence for Solar-Wind Charge-Exchange X-Ray Emission from the Earth's Magnetosheath
Yamaguchi, Hiroya; Mitsuda, Kazuhisa; Fujimoto, Ryuichi +7 more
We report an apparent detection of the C VI 4p to 1s transition line at 459eV, during a long-term enhancement (LTE) in the Suzaku north ecliptic pole observation of 2005 September 2. The observed line intensity is comparable to that of the C VI 2p to 1s line at 367eV. This is strong evidence for the charge-exchange process. In addition, O VII , O …
Iron and Nickel Line Diagnostics for the Galactic Center Diffuse Emission
Maeda, Yoshitomo; Takahashi, Tadayuki; Koyama, Katsuji +14 more
We have observed the diffuse X-ray emission from the Galactic Center (GC) using the X-ray Imaging Spectrometer (XIS) on Suzaku. The high-energy resolution and the low-background orbit provided excellent spectra of the GC diffuse X-rays (GCDX). The XIS found many emission lines in the GCDX near the energy of K-shell transitions of iron and nickel. …
The Suzaku High Resolution X-Ray Spectrometer
Ishida, Manabu; Kelley, Richard L.; Kilbourne, Caroline A. +41 more
The X-Ray Spectrometer (XRS) has been designed to provide the Suzaku Observatory with non-dispersive, high-resolution X-ray spectroscopy. As designed, the instrument covers the energy range 0.3 to 12keV, which encompasses the most diagnostically rich part of the X-ray band. The sensor consists of a 32-channel array of X-ray microcalorimeters, each…