Search Publications

Calibration of the AKARI Far-Infrared Imaging Fourier-Transform Spectrometer
DOI: 10.1093/pasj/62.5.1155 Bibcode: 2010PASJ...62.1155M

Nakagawa, Takao; Shirahata, Mai; Doi, Yasuo +16 more

The Far-Infrared Surveyor (FIS) onboard the AKARI satellite has a spectroscopic capability provided by a Fourier transform spectrometer (FIS-FTS). FIS-FTS is the first space-borne imaging FTS dedicated to far-infrared astronomical observations. We describe the calibration process of the FIS-FTS, and discuss its accuracy and reliability. The calibr…

2010 Publications of the Astronomical Society of Japan
AKARI ISO 7
Time-Resolved Spectral Variability of the Prompt Emission from GRB 070125 Observed with Suzaku/WAM
DOI: 10.1093/pasj/62.3.547 Bibcode: 2010PASJ...62..547O

Gandhi, Poshak; Yamaoka, Kazutaka; Fukazawa, Yasushi +12 more

Time-resolved spectral analyses of GRB 070125 with significant photon detections over the MeV regime using Suzaku/WAM data are reported. The prompt emission interval was divided into 10 time regions, and their spectra were reproduced by a Band function or a cutoff power-law model. The spectra show a complex evolution; a soft-hard-soft trend is see…

2010 Publications of the Astronomical Society of Japan
Suzaku 6
Spectroscopic Studies of Limb Spicules. I Radial and Turbulent Velocities
DOI: 10.1093/pasj/62.4.927 Bibcode: 2010PASJ...62..927S

Shoji, Makiko; Nishikawa, Takara; Kitai, Reizaburo +1 more

We made high-resolution spectroscopic observations of limb spicules in Hα using the Vertical Spectrograph of Domeless Solar Telescope at Hida Observatory. While more than half of the observed spicules have Gaussian line-profiles, some spicules have distinctly asymmetric profiles, which can be fitted to two Gaussian components. The faster component…

2010 Publications of the Astronomical Society of Japan
SOHO 5
A New Candidate of a Cluster of Galaxies, 2XMM J045637.2+522411
DOI: 10.1093/pasj/62.2.219 Bibcode: 2010PASJ...62..219Y

Ueno, Masaru; Koyama, Katsuji; Bamba, Aya +1 more

We present XMM-Newton and Suzaku results of an X-ray source, 2XMM J045637.2+522411, found during an observation of a galactic supernova remnant (SNR), G156.2+5.7. By comparing its radial profile with the point-spread function, we found that 2XMM J045637.2+522411 is an extended source. X-ray spectra exhibited a line-like structure at 5.7-5.8 keV. S…

2010 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 4
Suzaku Observations of the Supernova Remnant N23 in the Large Magellanic Cloud
DOI: 10.1093/pasj/62.5.1301 Bibcode: 2010PASJ...62.1301S

Ishida, Manabu; Bamba, Aya; Someya, Kentaro

X-ray emission from the supernova remnant N23 in the Large Magellanic Cloud (LMC) has been studied using the X-ray Imaging Spectrometer (XIS) onboard Suzaku. Thanks to a superior energy resolution of the XIS in the soft X-ray band, we resolved H-like and He-like Oxygen K$\alpha$

2010 Publications of the Astronomical Society of Japan
Suzaku 3
On the Relation between Surge Activities and a Photospheric Horizontal Velocity Field
DOI: 10.1093/pasj/62.4.921 Bibcode: 2010PASJ...62..921K

Kitai, Reizaburo

A photospheric horizontal velocity field was observed in an active region, NOAA 8375, which showed high Hα surge activities on 1998 November 6. From analyses of Hα images, the photospheric horizontal velocity field, and the magnetic field in and around the active region, we found the following: (1) Meso-granular or supergranular photospheric horiz…

2010 Publications of the Astronomical Society of Japan
SOHO 2
Modeling and Reproducibility of Suzaku HXD PIN/GSO Background
DOI: 10.1093/pasj/61.sp1.S17 Bibcode: 2009PASJ...61S..17F

Isobe, Naoki; Enoto, Teruaki; Yamaoka, Kazutaka +27 more

Suzaku Hard X-ray Detector (HXD) achieved the lowest background level than any other previously or currently operational missions sensitive in the energy range of 10--600keV, by utilizing PIN photodiodes and GSO scintillators mounted in BGO active shields to reject particle background and Compton-scattered events as much as possible. Because it do…

2009 Publications of the Astronomical Society of Japan
Suzaku 183
Energy Spectra of the Soft X-Ray Diffuse Emission in Fourteen Fields Observed with Suzaku
DOI: 10.1093/pasj/61.4.805 Bibcode: 2009PASJ...61..805Y

Fujimoto, Ryuichi; Yamasaki, Noriko Y.; Wang, Q. Daniel +8 more

The soft diffuse X-ray emission of twelve fields observed with Suzaku are presented together with two additional fields from previous analyses. All have galactic longitudes 65° < l < 295° to avoid contributions from the very bright diffuse source that extends at least 30° from the Galactic center. The surface brightnesses of the Suzaku nine …

2009 Publications of the Astronomical Society of Japan
Suzaku 163
Suzaku Observations of Abell 1795: Cluster Emission to r200
DOI: 10.1093/pasj/61.5.1117 Bibcode: 2009PASJ...61.1117B

Miller, Eric D.; Sanders, Jeremy S.; Hughes, John P. +10 more

We report Suzaku observations of the galaxy cluster Abell 1795 that extend to r_200 ~ 2 Mpc, the radius within which the mean cluster mass density is 200 times the cosmic critical density. These observations are the first to probe the state of the intracluster medium in this object at r > 1.3 Mpc. We sample two disjoint sectors in the cluster o…

2009 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 135
New CTI Correction Method for Spaced-Row Charge Injection of the Suzaku X-Ray Imaging Spectrometer
DOI: 10.1093/pasj/61.sp1.S9 Bibcode: 2009PASJ...61S...9U

Dotani, Tadayasu; Miller, Eric D.; Mori, Hideyuki +21 more

The charge transfer inefficiency (CTI) of the X-ray CCDs on board the Suzaku satellite (X-ray Imaging Spectrometers; XIS) has increased since the launch due to radiation damage, and the energy resolution has been degraded. To improve the CTI, we have applied a spaced-row charge injection (SCI) technique to the XIS in orbit; by injecting charges in…

2009 Publications of the Astronomical Society of Japan
Suzaku 94